Optical and X-ray observations of 3U 0614+09

Details Optical and X-ray observations of 3U 0614+09 Optical and X-ray observations of 3U 0614+09

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...193l..25d&link_type=abstract

Astrophysical Journal, vol. 193, Oct. 1, 1974, pt. 2, p. L25-L29.

Astronomy and Astrophysics

Astrophysics

30

Hot Stars, Stellar Spectrophotometry, Variable Stars, X Ray Sources, Emission Spectra, Photographic Plates, Ultraviolet Spectra, X Rays

Scientific paper

Based on positional agreement, ultraviolet excess, and spectroscopic peculiarity, the identification of the X-ray source 3U 0614+09 with a faint blue star, previously suggested by Murdin et al. (1974) as a candidate, is established. Four days of X-ray observations at 1-3 A failed to show evidence for significant variability or eclipses. The possibility that this object may be very similar to Sco X-1, but at a distance of 4-8 kpc, is discussed.

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