Possible detection of an extreme-ultraviolet source at 500 A

Details Possible detection of an extreme-ultraviolet source at 500 A Possible detection of an extreme-ultraviolet source at 500 A

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...219..585c&link_type=abstract

Astrophysical Journal, Part 1, vol. 219, Jan. 15, 1978, p. 585-588.

Astronomy and Astrophysics

Astronomy

6

Far Ultraviolet Radiation, Ultraviolet Astronomy, Apollo Soyuz Test Project, Astronomical Maps, Interstellar Matter, Position Errors, Satellite-Borne Instruments, Spaceborne Astronomy, X Ray Sources

Scientific paper

Evidence for an extreme-ultraviolet source in the constellation Pavo is
presented. The potential source, which was observed in the 500-780-A
band, has an intensity of 35 + or - 9 mJy. Positional overlap suggests
possible identification with the ultraviolet-intense star HD 192273
and/or the high-galactic-latitude X-ray source 3U 1959-69.

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