The optical counterpart of the X-ray transient EXO 2030+375

Details The optical counterpart of the X-ray transient EXO 2030+375 The optical counterpart of the X-ray transient EXO 2030+375

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...182l..55m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 182, no. 2, Aug. 1987, p. L55-L58.

Astronomy and Astrophysics

Astrophysics

25

B Stars, Early Stars, Stellar Spectrophotometry, Visible Spectrum, X Ray Sources, Infrared Spectra, Interstellar Extinction, Stellar Color

Scientific paper

The authors present CCD photometric observations of the error circle of the X-ray source EXO 2030+375. The X-ray position and the optical and infrared colours allow the identification of the transient source with a highly reddened (E(B-V) = 3.8) early type star. The optical candidate has photometric characteristics consistent with a Be/X-ray system located at a distance of 2 - 7 kpc.

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