X-ray observations of SU UMa throughout six outbursts
Abstract
We present RXTE observations covering six normal outbursts of the dwarf nova SU UMa, the prototype of its class. The outbursts showed consistent X-ray behaviour with the X-ray count rate dropping suddenly by a factor of 4, and with evidence for a half-day delay between the optical rise and the X-ray suppression. In contrast to SS Cygni, an X-ray flux increase at the beginning of outburst was not observed, although it is expected from boundary-layer models. The X-ray flux was high and decreasing during quiescence, in conflict with the disc instability model. The X-ray spectrum of SU UMa was softer in outburst than during quiescence, and it was consistent with constant reflection.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- March 2010
- DOI:
- 10.1111/j.1365-2966.2009.16009.x
- arXiv:
- arXiv:0911.2711
- Bibcode:
- 2010MNRAS.402.1816C
- Keywords:
-
- accretion;
- accretion discs;
- binaries: close;
- stars: individual: SU UMa;
- novae;
- cataclysmic variables;
- X-rays: stars;
- Astrophysics - High Energy Astrophysical Phenomena;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- 9 pages, 9 figures, 3 tables, Accepted for publication in MNRAS