EDP Sciences Journals List
Advanced Search
Free access article

Issue A&A
Volume 371, Number 3, June I 2001
Page(s) 1018 - 1023
Section Formation, structure and evolution of stars
DOI http://dx.doi.org/10.1051/0004-6361:20010417



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. Stella1

1  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 $\geq$ 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


What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.
  • If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
  • You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
  • You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.