First Stellar Abundances in NGC 6822 from VLT-UVES and Keck-HIRES Spectroscopy**Based on observations obtained from the UVES commissioning at the Very Large Telescope (Kueyen), European Southern Observatory, Paranal, Chile, and the W. M. Keck Observatory, Hawaii. Keck is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration, and was made possible by the generous financial support of the W. M. Keck Foundation.
The Astrophysical Journal American Astronomical Society 547:2 (2001) 765-776
The WR content of IC10 - first detection of WC9 stars in a low metallicity environment?*
Astronomy & Astrophysics EDP Sciences 366:2 (2001) l1-l4
Spectral evidence for a powerful compact jet from XTE J1118+480
(2001)
On the peak radio and X-ray emission from neutron star and black hole candidate X-ray transients
(2001)