Virtual Observatory based identification of AX J194939+2631 as a new cataclysmic variable (Research Note)

被引:4
作者
Zolotukhin, I. Yu [1 ,2 ,3 ]
Chilingarian, I. V. [2 ,4 ]
机构
[1] Observ Paris, LERMA, UMR 8112, F-75014 Paris, France
[2] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119992, Russia
[3] Observ Paris, VO Paris Data Ctr, F-75014 Paris, France
[4] Univ Strasbourg, CNRS, Observ Astron Strasbourg, UMR 7550m, F-67000 Strasbourg, France
关键词
novae; cataclysmic variables; X-rays: binaries; X-rays: individuals: AX J194939+2631; stars: individual: IPHAS J194938.39+263149.2; NORTHERN GALACTIC PLANE; H-ALPHA SURVEY; SKY SURVEY; EMISSION; CATALOG; IPHAS;
D O I
10.1051/0004-6361/201015563
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a new cataclysmic variable (CV) among unidentified objects from the ASCA Galactic Plane Survey made using the Virtual Observatory data mining. First, we identified AX J194939+2631 with IPHAS J194938.39+263149.2, the only prominent H alpha emitter among 400 sources in a 1 arcmin field of the IPHAS survey, then secured as a single faint X-ray source found in an archival Chandra dataset. Spectroscopic follow-up with the 3.5-m Calar Alto telescope confirmed its classification as a CV, possibly of magnetic nature. Our analysis suggests that AX J194939+2631 is a medium distance system (d approximate to 0.6 kpc) containing a late-K or early-M type dwarf as a secondary component and a partially disrupted accretion disc revealed by the double-peaked H alpha line. However, additional deep observations are needed to confirm our tentative classification of this object as an intermediate polar.
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