English

Virtual Observatory based identification of AX J194939+2631 as a new cataclysmic variable

High Energy Astrophysical Phenomena 2015-05-20 v1 Astrophysics of Galaxies Instrumentation and Methods for Astrophysics

Abstract

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 ~ 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.

Keywords

Cite

@article{arxiv.1010.3440,
  title  = {Virtual Observatory based identification of AX J194939+2631 as a new cataclysmic variable},
  author = {Ivan Zolotukhin and Igor Chilingarian},
  journal= {arXiv preprint arXiv:1010.3440},
  year   = {2015}
}

Comments

5 pages, 5 figures, 2 tables, accepted to Astronomy and Astrophysics

R2 v1 2026-06-21T16:29:41.170Z