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

Astronomy and Astrophysics – Astronomy

Scientific paper

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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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