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A&A 371, 1018-1023 (2001)
DOI: 10.1051/0004-6361:20010417
The identification of the optical/IR counterpart of the 29.5-s transient X-ray pulsar GS 1843+009
G. L. Israel1, I. Negueruela2, 3, S. Campana4, S. Covino4, A. Di Paola1, D. H. Maxwell5, A. J. Norton5, R. Speziali1, F. Verrecchia6 and L. Stella11 Osservatorio Astronomico di Roma, Via Frascati 33, 00040 Monteporzio Catone, Italy
2 Observatoire Astronomique de Strasbourg, 11 rue de l'Université, 67000 Strasbourg, France
3 SAX Science Data Center, ASI c/o Telespazio, via Corcolle 19, 00131 Roma, Italy
4 Osservatorio Astronomico di Brera, Via E. Bianchi 46, 23807 Merate, Italy
5 Dept. of Physics & Astronomy, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK
6 Dipartimento di Fisica, Università degli Studi "La Sapienza", Piazza A. Moro 5, 00185 Roma, Italy
(Received 21 December 2000 / Accepted 19 March 2001 )
Abstract
We report on the identification of the optical/IR counterpart
of the 29.5-s transient X-ray pulsar GS 1843+009.
We re-analysed an archival ROSAT HRI observation of GS 1843+009 obtaining a new
refined position. The optical and IR follow-up
observations carried out for the new error circle allowed us to find
a relatively faint (V=20.9) and variable early type reddened star
(V-R=2.1). The
optical spectra show the Balmer and Paschen series in emission, while the
IR observations confirm the presence of a flux excess (H=13.2,
J-H=0.54), suggesting that the star is surrounded by a
circumstellar envelope.
Spectroscopic and photometric data together indicate a B0-B2 IV-Ve
spectral-type star located at a distance of
10 kpc confirming
the Be-star/X-ray binary nature of GS 1843+009.
Key words: stars: individual: -- GS 1843+009; 1BMW J184536.8+005148 -- binaries: general -- stars: pulsars: general -- stars: emission-line, Be -- X-rays: stars
Offprint request: G. L. Israel, Gianluca.Israel@oar.mporzio.astro.it
SIMBAD Objects
© ESO 2001
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