Copernicus observations of Theta-2 OriA, a proposed optical counterpart of the X-ray source 4U 0531-05

Details Copernicus observations of Theta-2 OriA, a proposed optical counterpart of the X-ray source 4U 0531-05 Copernicus observations of Theta-2 OriA, a proposed optical counterpart of the X-ray source 4U 0531-05

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....75...61b&link_type=abstract

Astronomy and Astrophysics, vol. 75, no. 1-2, May 1979, p. 61-72.

Astronomy and Astrophysics

Astrophysics

10

Binary Stars, Line Spectra, Stellar Mass Ejection, X Ray Sources, Absorption Spectra, Fine Structure, Flare Stars, Oao 3, Spaceborne Telescopes, Spectroscopic Telescopes, Stellar Mass Accretion, Stellar Radiation, Stellar Spectra, T Tauri Stars

Scientific paper

The binary system Theta-2 OriA, physical member of the Ori Ic subgroup of the I Orionis association, falls within the error box of the X-ray source 4U 0531-05, as observed by Uhuru, Ariel V and ANS satellites. An examination of the present observational material indicates that there are no strong objections, at this stage, to Theta-2 OriA as the possible optical counterpart of 4U 0531-05.

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