Far-Ultraviolet Stellar Photometry

Details Far-Ultraviolet Stellar Photometry Far-Ultraviolet Stellar Photometry

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...183.1702s&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #17.02; Bulletin of the American Astronomical Society, Vol. 25, p.1317

Astronomy and Astrophysics

Astronomy

Scientific paper

During a shuttle flight in May, 1991, wide field images were obtained for 12 star fields with the NRL far-ultraviolet cameras. These cameras provide sensitivity bands with effective wavelengths of lambda eff = 1367 Angstroms and lambda eff = 1702 Angstroms. The properties of the resulting magnitude system will be described and compared with previous photometry from the OAO2, ANS and TD1 satellites. Results from several fields in the vicinity of the galactic center will be discussed.

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