The optical/IR counterpart to the newly-discovered X-ray source EXO 2030+375

Details The optical/IR counterpart to the newly-discovered X-ray source EXO 2030+375 The optical/IR counterpart to the newly-discovered X-ray source EXO 2030+375

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.232..865c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 232, June 15, 1988, p. 865-871. SERC-supported research

Astronomy and Astrophysics

Astronomy

33

Astronomical Photometry, Infrared Spectra, Pulsars, Visible Spectrum, X Ray Sources, Companion Stars, Doppler Effect, Error Analysis, Exosat Satellite

Scientific paper

Near-infrared (JHK) photometry and 5000 - 7000 Å optical spectrometry have been obtained of possible counterparts of the newly discovered X-ray source, EXO 2030+375. A study of the EXOSAT error circle has revealed two possible candidates. Using the combined optical-to-IR data the most probable counterpart has been identified from the shape of the spectrum, and from the LX/Lopt ratio. The system bears certain similarities to V0332+53.

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