Galaxy and Magellanic Clouds OB and WR stars (Robert+, 2003)

Details Galaxy and Magellanic Clouds OB and WR stars (Robert+, 2003) Galaxy and Magellanic Clouds OB and WR stars (Robert+, 2003)

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..21440021r&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/144/21. Originally published in: 2003ApJS..144...21R

Physics

Stars: Early-Type, Mk Spectral Classification, Photometry: Ubv

Scientific paper

Our far-UV libraries contain spectra of OB and Wolf-Rayet (WR) stars collected with FUSE mainly during its first cycle (1999 December to 2000 December). The FUSE instrument provides redundant wavelength coverage by means of eight independent spectra, each covering a ~100{AA} region between 905 and 1187{AA} at a resolving power of ~20,000. A detailed description of FUSE can be found in Moos et al. (2000ApJ...538L...1M) and Sahnow et al. (2000ApJ...538L...7S).
(3 data files).

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