Chris B. Brook

Structure, Kinematics, and Chemical Enrichment Patterns after Major Gas-Rich Disc-Disc Mergers (2009)

Richard, Simon, Brook, Chris B., Martel, Hugo, Kawata, Daisuke, Gibson, Brad K., Sanchez-Blazquez, Patricia

We used an N-body smoothed particle hydrodynamics algorithm, with a detailed treatment of star formation, supernovae feedback, and chemical enrichment, to perform eight simulations of mergers between...

Chemodynamical analysis of bulge stars for simulated disc galaxies (2009)

Rahimi, A., Kawata, D., Brook, Chris B., Gibson, Brad K.

We analyse the kinematics and chemistry of the bulge stars of two simulated disc galaxies using our chemodynamical galaxy evolution code GCD+. First we compare stars that are born inside the galaxy...

Orbital Eccentricity as a probe of Thick Disk Formation Scenarios (2009)

Sales, Laura V., Helmi, Amina, Abadi, Mario G., Brook, Chris B., Gomez, Facundo A., Roskar, Rok, ...

We study the orbital properties of stars in four (published) simulations of thick disks formed by: i) accretion from disrupted satellites, ii) heating of a pre-existing thin disk by a minor merger,...

The Dual Origin of Stellar Halos (2009)

Zolotov, Adi, Willman, Beth, Brooks, Alyson M., Governato, Fabio, Brook, Chris B., Hogg, David W., ...

We investigate the formation of the stellar halos of four simulated disk galaxies using high-resolution, cosmological SPH + N-body simulations. These simulations include a self-consistent treatment...

The Dual Origin of Stellar Halos (2009)

Zolotov, Adi, Willman, Beth, Brooks, Alyson M., Governato, Fabio, Brook, Chris B., Hogg, David W., ...

We investigate the formation of the stellar halos of four simulated disk galaxies using high resolution, cosmological SPH + N-Body simulations. These simulations include a self-consistent treatment...

Hydrodynamical Adaptive Mesh Refinement Simulations of Disk Galaxies (2008)

Gibson, Brad K., Courty, Stephanie, Sanchez-Blazquez, Patricia, Teyssier, Romain, House, Elisa L., Brook, Chris B., ...

To date, fully cosmological hydrodynamic disk simulations to redshift zero have only been undertaken with particle-based codes, such as GADGET, Gasoline, or GCD+. In light of the (supposed)...

The Formation of Polar Disk Galaxies (2008)

Brook, Chris B., Governato, Fabio, Quinn, Thomas, Wadsley, James, Brooks, Alyson M., Willman, Beth, ...

Polar Ring Galaxies, such as NGC4650A, are a class of galaxy which have two kinematically distinct components that are inclined by almost 90 degrees to each other. These striking galaxies challenge...

The Spatial Distribution of the Galactic First Stars. I. High-Resolution N-Body Approach (2007)

Scannapieco, Evan, Kawata, Daisuke, Brook, Chris B., Schneider, Raffaella, Ferrara, Andrea, Gibson, Brad K.

We study the spatial distribution of Galactic metal-free stars by combining an extremely high-resolution (7.8 X 10^5 solar masses per particle) Cold Dark Matter N-body simulation of the Milky-Way...

Two disk components from a gas-rich disk-disk merger (2007)

Brook, Chris B., Richard, Simon, Kawata, Daisuke, Martel, Hugo, Gibson, Brad K.

We employ N-body, smoothed particle hydrodynamic simulations, including detailed treatment of chemical enrichment, to follow a gas-rich merger that results in a galaxy with disk morphology. We trace...

Two disk components from a gas-rich disk-disk merger (2007)

Brook, Chris B., Richard, Simon, Kawata, Daisuke, Martel, Hugo, Gibson, Brad K.

We employ N-body, smoothed particle hydrodynamic simulations, including detailed treatment of chemical enrichment, to follow a gas-rich merger that results in a galaxy with disk morphology. We trace...

Two disk components from a gas-rich disk-disk merger (2007)

Brook, Chris B., Richard, Simon, Kawata, Daisuke, Martel, Hugo, Gibson, Brad K.

We employ N-body, smoothed particle hydrodynamic simulations, including detailed treatment of chemical enrichment, to follow a gas-rich merger that results in a galaxy with disk morphology. We trace...

Two disk components from a gas-rich disk-disk merger (2007)

Brook, Chris B., Richard, Simon, Kawata, Daisuke, Martel, Hugo, Gibson, Brad K.

We employ N-body, smoothed particle hydrodynamic simulations, including detailed treatment of chemical enrichment, to follow a gas-rich merger that results in a galaxy with disk morphology. We trace...

Two disk components from a gas-rich disk-disk merger (2007)

Brook, Chris B., Richard, Simon, Kawata, Daisuke, Martel, Hugo, Gibson, Brad K.

We employ N-body, smoothed particle hydrodynamic simulations, including detailed treatment of chemical enrichment, to follow a gas-rich merger that results in a galaxy with disk morphology. We trace...

The Spatial Distribution of the Galactic First Stars II: SPH Approach (2006)

Brook, Chris B., Kawata, Daisuke, Scannapieco, Evan, Martel, Hugo, Gibson, Brad K.

We use cosmological, chemo-dynamical, smoothed particle hydrodynamical simulations of Milky-Way-analogue galaxies to find the expected present-day distributions of both metal-free stars that formed...

The Spatial Distribution of the Galactic First Stars I: High-Resolution N-body Approach (2006)

Scannapieco, Evan, Kawata, Daisuke, Brook, Chris B., Schneider, Raffaella, Ferrara, Andrea, Gibson, Brad K.

We study the spatial distribution of Galactic metal-free stars by combining an extremely high-resolution (7.8 X 10^5 solar masses per particle) Cold Dark Matter N-body simulation of the Milky-Way...

Disk evolution since z-1 in a CDM universe (2006)

Brook, Chris B., Kawata, Daisuke, Martel, Hugo, Gibson, Brad K., Bailin, Jeremy

Increasingly large populations of disk galaxies are now being observed at increasingly high redshifts, providing new constraints on our knowledge of how such galaxies evolve. Are these observations...

Disk evolution since z-1 in a CDM universe (2006)

Brook, Chris B., Kawata, Daisuke, Martel, Hugo, Gibson, Brad K., Bailin, Jeremy

Increasingly large populations of disk galaxies are now being observed at increasingly high redshifts, providing new constraints on our knowledge of how such galaxies evolve. Are these observations...

Disk evolution since z-1 in a CDM universe (2006)

Brook, Chris B., Kawata, Daisuke, Martel, Hugo, Gibson, Brad K., Bailin, Jeremy

Increasingly large populations of disk galaxies are now being observed at increasingly high redshifts, providing new constraints on our knowledge of how such galaxies evolve. Are these observations...

Disk evolution since z-1 in a CDM universe (2006)

Brook, Chris B., Kawata, Daisuke, Martel, Hugo, Gibson, Brad K., Bailin, Jeremy

Increasingly large populations of disk galaxies are now being observed at increasingly high redshifts, providing new constraints on our knowledge of how such galaxies evolve. Are these observations...

Disk evolution since z-1 in a CDM universe (2006)

Brook, Chris B., Kawata, Daisuke, Martel, Hugo, Gibson, Brad K., Bailin, Jeremy

Increasingly large populations of disk galaxies are now being observed at increasingly high redshifts, providing new constraints on our knowledge of how such galaxies evolve. Are these observations...

Gas Rich Mergers in Disk Formation (2005)

Brook, Chris B., Veilleux, Vincent, Kawata, Daisuke, Martel, Hugo, Gibson, Brad K.

In order to explain disk galaxy formation within the hierarchical structure formation, it seems that gas rich mergers must play an important role. We review here our previous studies which have shown...

The Stellar Halo Metallicity - Luminosity Relationship for Spiral Galaxies (2005)

Renda, Agostino, Gibson, Brad K., Mouhcine, Mustapha, Ibata, Rodrigo A., Kawata, Daisuke, Flynn, Chris, ...

The stellar halos of spiral galaxies bear important chemo-dynamical signatures of galaxy formation. We present here the analysis of 89 semi-cosmological spiral galaxy simulations, spanning ~ 4...

Internal Alignment of the Halos of Disk Galaxies in Cosmological Hydrodynamic Simulations (2005)

Bailin, Jeremy, Kawata, Daisuke, Gibson, Brad K., Steinmetz, Matthias, Navarro, Julio F., Brook, Chris B., ...

Seven cosmological hydrodynamic simulations of disk galaxy formation are analyzed to determine the alignment of the disk within the dark matter halo and the internal structure of the halo. We find...

The Emergence of the Thick Disk in a CDM Universe II: Colors and Abundance Patterns (2005)

Brook, Chris B., Gibson, Brad K., Martel, Hugo, Kawata, Daisuke

The recently emerging conviction that thick disks are prevalent in disk galaxies, and their seemingly ubiquitous old ages, means that the formation of the thick disk, perhaps more than any other...

The emergence of the thick disk in a CDM universe. II. Colours and abundance patterns (2005)

Brook, Chris B., Gibson, Brad K., Martel, Hugo, Kawata, Daisuke

The recently emerging conviction that thick disks are prevalent in disk galaxies, and their seemingly ubiquitous old ages, means that the formation of the thick disk, perhaps more than any other...

The stellar halo metallicity-luminosity relationship for spiral galaxies (2005)

Renda, Agostino, Gibson, Brad K., Mouhcine, Mustapha, Ibata, Rodrigo A., Kawata, Daisuke, Flynn, Chris, ...

The stellar haloes of spiral galaxies bear important chemodynamical signatures of galaxy formation. We present here the analysis of 89 semi-cosmological spiral galaxy simulations, spanning ~4 mag in...

Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations (2005)

Bailin, Jeremy, Kawata, Daisuke, Gibson, Brad K., Steinmetz, Matthias, Navarro, Julio F., Brook, Chris B., ...

Seven cosmological hydrodynamic simulations of disk galaxy formation are analyzed to determine the alignment of the disk within the dark matter halo and the internal structure of the halo. We find...

Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations (2005)

Bailin, Jeremy, Kawata, Daisuke, Gibson, Brad K., Steinmetz, Matthias, Navarro, Julio F., Brook, Chris B., ...

Seven cosmological hydrodynamic simulations of disk galaxy formation are analyzed to determine the alignment of the disk within the dark matter halo and the internal structure of the halo. We find...

The stellar halo metallicity-luminosity relationship for spiral galaxies (2005)

Renda, Agostino, Gibson, Brad K., Mouhcine, Mustapha, Ibata, Rodrigo A., Kawata, Daisuke, Flynn, Chris, ...

The stellar haloes of spiral galaxies bear important chemodynamical signatures of galaxy formation. We present here the analysis of 89 semi-cosmological spiral galaxy simulations, spanning ~4 mag in...

The emergence of the thick disk in a CDM universe. II. Colours and abundance patterns (2005)

Brook, Chris B., Gibson, Brad K., Martel, Hugo, Kawata, Daisuke

The recently emerging conviction that thick disks are prevalent in disk galaxies, and their seemingly ubiquitous old ages, means that the formation of the thick disk, perhaps more than any other...

Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations (2005)

Bailin, Jeremy, Kawata, Daisuke, Gibson, Brad K., Steinmetz, Matthias, Navarro, Julio F., Brook, Chris B., ...

Seven cosmological hydrodynamic simulations of disk galaxy formation are analyzed to determine the alignment of the disk within the dark matter halo and the internal structure of the halo. We find...

The stellar halo metallicity-luminosity relationship for spiral galaxies (2005)

Renda, Agostino, Gibson, Brad K., Mouhcine, Mustapha, Ibata, Rodrigo A., Kawata, Daisuke, Flynn, Chris, ...

The stellar haloes of spiral galaxies bear important chemodynamical signatures of galaxy formation. We present here the analysis of 89 semi-cosmological spiral galaxy simulations, spanning ~4 mag in...

The emergence of the thick disk in a CDM universe. II. Colours and abundance patterns (2005)

Brook, Chris B., Gibson, Brad K., Martel, Hugo, Kawata, Daisuke

The recently emerging conviction that thick disks are prevalent in disk galaxies, and their seemingly ubiquitous old ages, means that the formation of the thick disk, perhaps more than any other...

Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations (2005)

Bailin, Jeremy, Kawata, Daisuke, Gibson, Brad K., Steinmetz, Matthias, Navarro, Julio F., Brook, Chris B., ...

Seven cosmological hydrodynamic simulations of disk galaxy formation are analyzed to determine the alignment of the disk within the dark matter halo and the internal structure of the halo. We find...

The stellar halo metallicity-luminosity relationship for spiral galaxies (2005)

Renda, Agostino, Gibson, Brad K., Mouhcine, Mustapha, Ibata, Rodrigo A., Kawata, Daisuke, Flynn, Chris, ...

The stellar haloes of spiral galaxies bear important chemodynamical signatures of galaxy formation. We present here the analysis of 89 semi-cosmological spiral galaxy simulations, spanning ~4 mag in...

The emergence of the thick disk in a CDM universe. II. Colours and abundance patterns (2005)

Brook, Chris B., Gibson, Brad K., Martel, Hugo, Kawata, Daisuke

The recently emerging conviction that thick disks are prevalent in disk galaxies, and their seemingly ubiquitous old ages, means that the formation of the thick disk, perhaps more than any other...

The stellar halo metallicity-luminosity relationship for spiral galaxies (2005)

Renda, Agostino, Gibson, Brad K., Mouhcine, Mustapha, Ibata, Rodrigo A., Kawata, Daisuke, Flynn, Chris, ...

The stellar haloes of spiral galaxies bear important chemodynamical signatures of galaxy formation. We present here the analysis of 89 semi-cosmological spiral galaxy simulations, spanning ~4 mag in...

Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations (2005)

Bailin, Jeremy, Kawata, Daisuke, Gibson, Brad K., Steinmetz, Matthias, Navarro, Julio F., Brook, Chris B., ...

Seven cosmological hydrodynamic simulations of disk galaxy formation are analyzed to determine the alignment of the disk within the dark matter halo and the internal structure of the halo. We find...

The emergence of the thick disk in a CDM universe. II. Colours and abundance patterns (2005)

Brook, Chris B., Gibson, Brad K., Martel, Hugo, Kawata, Daisuke

The recently emerging conviction that thick disks are prevalent in disk galaxies, and their seemingly ubiquitous old ages, means that the formation of the thick disk, perhaps more than any other...

The stellar halo metallicity-luminosity relationship for spiral galaxies (2005)

Renda, Agostino, Gibson, Brad K., Mouhcine, Mustapha, Ibata, Rodrigo A., Kawata, Daisuke, Flynn, Chris, ...

The stellar haloes of spiral galaxies bear important chemodynamical signatures of galaxy formation. We present here the analysis of 89 semi-cosmological spiral galaxy simulations, spanning ~4 mag in...

The Emergence of the Thick Disk in a CDM Universe (2004)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Freeman, Ken C.

The disk galaxy simulated using our chemo-dynamical galaxy formation code, GCD+, is shown to have a thick disk component. This is evidenced by the velocity dispersion versus age relation for solar...

The emergence of the thick disk in a cold dark matter universe (2004)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Freeman, Ken C.

The disk galaxy simulated using our chemodynamic galaxy formation code, GCD+, is shown to have a thick-disk component. This is evidenced by the velocity dispersion versus age relation for solar...

Stellar halo constraints on simulated late-type galaxies (2004)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

How do late-type spiral galaxies form within the context of a cold dark matter cosmology? We contrast N-body, smoothed particle hydrodynamical simulations of galaxy formation that employ two...

Photometric properties of white dwarf dominated halos (2004)

Lee, Hyun-Chul, Gibson, Brad K., Fenner, Yeshe, Brook, Chris B., Kawata, Daisuke, Renda, Agostino, ...

Using stellar population synthesis techniques, we explore the photometric signatures of white dwarf progenitor dominated galactic halos, in order to constrain the fraction of halo mass that may be...

Photometric properties of white dwarf dominated halos (2004)

Lee, Hyun-Chul, Gibson, Brad K., Fenner, Yeshe, Brook, Chris B., Kawata, Daisuke, Renda, Agostino, ...

Using stellar population synthesis techniques, we explore the photometric signatures of white dwarf progenitor dominated galactic halos, in order to constrain the fraction of halo mass that may be...

The emergence of the thick disk in a cold dark matter universe (2004)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Freeman, Ken C.

The disk galaxy simulated using our chemodynamic galaxy formation code, GCD+, is shown to have a thick-disk component. This is evidenced by the velocity dispersion versus age relation for solar...

Stellar halo constraints on simulated late-type galaxies (2004)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

How do late-type spiral galaxies form within the context of a cold dark matter cosmology? We contrast N-body, smoothed particle hydrodynamical simulations of galaxy formation that employ two...

Chemo-dynamical simulations of the Milky Way (2004)

Brook, Chris B.

Using a state of the art galaxy formation software package, GCD+, we model the formation and evolution of galaxies which resemble our own Galaxy, the Milky Way. The simulations include gravity, gas...

Photometric properties of white dwarf dominated halos (2004)

Lee, Hyun-Chul, Gibson, Brad K., Fenner, Yeshe, Brook, Chris B., Kawata, Daisuke, Renda, Agostino, ...

Using stellar population synthesis techniques, we explore the photometric signatures of white dwarf progenitor dominated galactic halos, in order to constrain the fraction of halo mass that may be...

The emergence of the thick disk in a cold dark matter universe (2004)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Freeman, Ken C.

The disk galaxy simulated using our chemodynamic galaxy formation code, GCD+, is shown to have a thick-disk component. This is evidenced by the velocity dispersion versus age relation for solar...

Stellar halo constraints on simulated late-type galaxies (2004)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

How do late-type spiral galaxies form within the context of a cold dark matter cosmology? We contrast N-body, smoothed particle hydrodynamical simulations of galaxy formation that employ two...

Chemo-dynamical simulations of the Milky Way (2004)

Brook, Chris B.

Using a state of the art galaxy formation software package, GCD+, we model the formation and evolution of galaxies which resemble our own Galaxy, the Milky Way. The simulations include gravity, gas...

The emergence of the thick disk in a cold dark matter universe (2004)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Freeman, Ken C.

The disk galaxy simulated using our chemodynamic galaxy formation code, GCD+, is shown to have a thick-disk component. This is evidenced by the velocity dispersion versus age relation for solar...

Stellar halo constraints on simulated late-type galaxies (2004)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

How do late-type spiral galaxies form within the context of a cold dark matter cosmology? We contrast N-body, smoothed particle hydrodynamical simulations of galaxy formation that employ two...

Photometric properties of white dwarf dominated halos (2004)

Lee, Hyun-Chul, Gibson, Brad K., Fenner, Yeshe, Brook, Chris B., Kawata, Daisuke, Renda, Agostino, ...

Using stellar population synthesis techniques, we explore the photometric signatures of white dwarf progenitor dominated galactic halos, in order to constrain the fraction of halo mass that may be...

Chemo-dynamical simulations of the Milky Way (2004)

Brook, Chris B.

Using a state of the art galaxy formation software package, GCD+, we model the formation and evolution of galaxies which resemble our own Galaxy, the Milky Way. The simulations include gravity, gas...

Chemo-dynamical simulations of the Milky Way (2004)

Brook, Chris B.

Using a state of the art galaxy formation software package, GCD+, we model the formation and evolution of galaxies which resemble our own Galaxy, the Milky Way. The simulations include gravity, gas...

The emergence of the thick disk in a cold dark matter universe (2004)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Freeman, Ken C.

The disk galaxy simulated using our chemodynamic galaxy formation code, GCD+, is shown to have a thick-disk component. This is evidenced by the velocity dispersion versus age relation for solar...

Stellar halo constraints on simulated late-type galaxies (2004)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

How do late-type spiral galaxies form within the context of a cold dark matter cosmology? We contrast N-body, smoothed particle hydrodynamical simulations of galaxy formation that employ two...

Photometric properties of white dwarf dominated halos (2004)

Lee, Hyun-Chul, Gibson, Brad K., Fenner, Yeshe, Brook, Chris B., Kawata, Daisuke, Renda, Agostino, ...

Using stellar population synthesis techniques, we explore the photometric signatures of white dwarf progenitor dominated galactic halos, in order to constrain the fraction of halo mass that may be...

Chemo-dynamical simulations of the Milky Way (2004)

Brook, Chris B.

Using a state of the art galaxy formation software package, GCD+, we model the formation and evolution of galaxies which resemble our own Galaxy, the Milky Way. The simulations include gravity, gas...

Stellar Halo Constraints on Simulated Late Type Galaxies (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

How do late type spiral galaxies form within the context of a CDM cosmology? We contrast N-body, smoothed particle hydrodynamical simulations of galaxy formation which employ two different supernova...

Simulating a White Dwarf-dominated Galactic Halo (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K.

Observational evidence has suggested the possibility of a Galactic halo which is dominated by white dwarfs (WDs). While debate continues concerning the interpretation of this evidence, it is clear...

Galactic Halo Stars in Phase Space :A Hint of Satellite Accretion? (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

The present day chemical and dynamical properties of the Milky Way bear the imprint of the Galaxy's formation and evolutionary history. One of the most enduring and critical debates surrounding...

Simulating a white dwarf dominated Galactic halo (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K.

Observational evidence has suggested the possibility of a Galactic halo dominated by white dwarfs (WDs). While debate continues concerning the interpretation of this evidence, it is clear that an...

Galactic halo stars in phase space: a hint of satellite accretion? (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

The present-day chemical and dynamical properties of the Milky Way bear the imprint of the Galaxy's formation and evolutionary history. One of the most enduring and critical debates surrounding...

On the origin of high-eccentricity halo stars (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

The present-day chemical and dynamical properties of the Milky Way aresignatures of the Galaxy's formation and evolution. Using a selfconsistent chemodynamical evolution code we examine these...

Simulating a white dwarf dominated Galactic halo (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K.

Observational evidence has suggested the possibility of a Galactic halo dominated by white dwarfs (WDs). While debate continues concerning the interpretation of this evidence, it is clear that an...

On the origin of high-eccentricity halo stars (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

The present-day chemical and dynamical properties of the Milky Way aresignatures of the Galaxy's formation and evolution. Using a selfconsistent chemodynamical evolution code we examine these...

Galactic halo stars in phase space: a hint of satellite accretion? (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

The present-day chemical and dynamical properties of the Milky Way bear the imprint of the Galaxy's formation and evolutionary history. One of the most enduring and critical debates surrounding...

Simulating a white dwarf dominated Galactic halo (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K.

Observational evidence has suggested the possibility of a Galactic halo dominated by white dwarfs (WDs). While debate continues concerning the interpretation of this evidence, it is clear that an...

On the origin of high-eccentricity halo stars (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

The present-day chemical and dynamical properties of the Milky Way aresignatures of the Galaxy's formation and evolution. Using a selfconsistent chemodynamical evolution code we examine these...

Galactic halo stars in phase space: a hint of satellite accretion? (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

The present-day chemical and dynamical properties of the Milky Way bear the imprint of the Galaxy's formation and evolutionary history. One of the most enduring and critical debates surrounding...

On the origin of high-eccentricity halo stars (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

The present-day chemical and dynamical properties of the Milky Way aresignatures of the Galaxy's formation and evolution. Using a selfconsistent chemodynamical evolution code we examine these...

Simulating a white dwarf dominated Galactic halo (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K.

Observational evidence has suggested the possibility of a Galactic halo dominated by white dwarfs (WDs). While debate continues concerning the interpretation of this evidence, it is clear that an...

Galactic halo stars in phase space: a hint of satellite accretion? (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

The present-day chemical and dynamical properties of the Milky Way bear the imprint of the Galaxy's formation and evolutionary history. One of the most enduring and critical debates surrounding...

On the origin of high-eccentricity halo stars (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

The present-day chemical and dynamical properties of the Milky Way aresignatures of the Galaxy's formation and evolution. Using a selfconsistent chemodynamical evolution code we examine these...

Simulating a white dwarf dominated Galactic halo (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K.

Observational evidence has suggested the possibility of a Galactic halo dominated by white dwarfs (WDs). While debate continues concerning the interpretation of this evidence, it is clear that an...

Galactic halo stars in phase space: a hint of satellite accretion? (2003)

Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Flynn, Chris

The present-day chemical and dynamical properties of the Milky Way bear the imprint of the Galaxy's formation and evolutionary history. One of the most enduring and critical debates surrounding...

Type Ia Supernovae and the Value of the Hubble Constant (2000)

Gibson, Brad K., Brook, Chris B.

The methodology involved in deriving the Hubble Constant via the calibration of the corrected peak luminosities of Type Ia supernovae (SNe) is reviewed. We first present a re-analysis of the...