Negueruela, I.; Reig, P. and Clark, J. S.
The nature of 1WGA J1958.2+3232: A new intermediate polar.
Astronomy and Astrophysics, 354(1) L29-L32.
Full text available as:
We present low and intermediate resolution spectroscopy of the optical counterpart to the recently discovered pulsating X-ray source 1WGA J1958.2+3232. The presence of strong HI , HeI and HeII emission lines together with the absence of absorption features rules out the possibility that the object is a massive star, as had recently been suggested. The observed X-ray and optical characteristics are consistent with the object being an intermediate polar. The double-peaked structure of the emission lines indicates that an accretion disc is present.
|External Project Funding Details:
|Funded Project Name||Project ID||Funding Body|
|Not Set||Not Set||European Union Training and Mobility of Researchers Network [grant number ERBFMRX/CT98/0195]|
||stars: individual, 1WGA J1958.2+3232; stars: binaries, close; stars: novae, cataclysmic variables; book reviews; X-rays: stars
||Science > Physical Sciences
|Interdisciplinary Research Centre:
||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
||23 Mar 2009 13:40
||12 Feb 2012 20:34
Actions (login may be required)