High-resolution (R ≈ 100,000), high signal-to-noise spectra of M71 giants have been obtained with High Resolution Echelle Spectrometer at the Keck I telescope in order to measure their Mg isotopic...
Metal-poor globular clusters of the galactic bulge (2009)
Barbuy, B., Dias, B., Alves-Brito, A., Zoccali, M., Minniti, D., Meléndez, J., ...
Chemical similarities between galactic bulge and local thick disk red giant stars (2008)
Meléndez, J., Asplund, M., Alves-Brito, A., Cunha, K., Barbuy, B., Bessell, M. S., ...
Abundances in the galactic bulge (2008)
Barbuy, B., Alves-Brito, A., Ortolani, S., Zoccali, M., Hill, V., Meléndez, J., ...
Precise radial velocities of giant stars. III. Spectroscopic stellar parameters (2007)
Context: A radial velocity survey of about 380 G and K giant stars is ongoing at Lick observatory. For each star we have a high signal to noise ratio template spectrum, which we use to determine...
VLT-UVES abundance analysis of four giants in NGC 6553 (2006)
Alves Brito, A., Barbuy, B., Zoccali, M., Minniti, D., Ortolani, S., Hill, V., ...
Context. Metal-rich globular clusters trace the formation of bulges. Abundance ratios in the metal-rich globular clusters such as NGC 6553 can constrain the formation timescale of the Galactic bulge....
Dueñas-Gonzalez, A., Lopez-Graniel, C., Gonzalez, A., Reyes, M., Mota, A., Muñoz, D., ...
Background Cisplatin-based chemoradiation for locally advanced cervical carcinoma is now the standard of care for most patients with cervical carcinoma However, induction chemotherapy followed by...