Andrea Moneti

The Evolution of Circumstellar Disks: Lessons from the VLT and ISO (2001)

Brandner, Wolfgang, Potter, Dan, Sheppard, Scott S., Moneti, Andrea, Zinnecker, Hans

There is strong evidence that the planets in the solar system evolved from a disk-shaped solar nebula ~4.56 Gyr ago. By studying young stars in various evolutionary stages, one aims at tracing back...

HST/NICMOS detection of a partially embedded, intermediate-mass pre-main-sequence population in the 30 Doradus Nebula (2001)

Brandner, Wolfgang, Grebel, Eva K., Barba, Rodolfo H., Walborn, Nolan R., Moneti, Andrea

We present the detection of an intermediate-mass pre-main-sequence population embedded in the nebular filaments surrounding the 30 Doradus region in the Large Magellanic Cloud (LMC) using HST/NICMOS....

Cold H2O and CO ice and gas toward the Galactic Center (2000)

Moneti, Andrea, Cernicharo, Jose, Pardo, Juan Ramon

We present observations of CO, 13CO and of H2O in the middle and far-infrared taken with the ISO-SWS and ISO-LWS spectrometers toward two positions in the Galactic Center region (Sgr A* and GCS-3)....

Cold H2O and CO ice and gas toward the Galactic Center (2000)

Moneti, Andrea, Cernicharo, José, Pardo Carrión, Juan Ramón

We present observations of CO, 13CO and of H2O in the middle and far-infrared taken with the ISO-SWS and ISO-LWS spectrometers toward two positions in the Galactic Center region (Sgr A* and GCS-3)....

Spectroscopy of the Pistol and Quintuplet stars in the galactic centre (1998)

Moneti, Andrea, Blommaert, Joris, Najarro, Francisco, Figer, Donald, Stolovy, Susan

"Spectroscopy of the Pistol and Quintuplet Stars in the Galactic Centre," Proceedings of The Universe as seen by ISO Conference. Held at UNESCO: Paris, France: 20-23 October 1998. AND Also archived...

Multiplicity among T Tauri stars in OB and T associations: Implications for binary star formation (1995)

Brandner, Wolfgang, Alcala, Juan M., Kunkel, Michael, Moneti, Andrea, Zinnecker, Hans

We present first results of a survey for companions among X-ray selected pre-main sequence stars, most of them being weak-line T Tauri stars (WTTS). These T Tauri stars have been identified in the...