Continuing X-ray Emission of Nova Vul 2007

Drake, J. J.; Page, K.; Osborne, J.; Beardmore, A.; Ness, J.-U.; Starrfield, S.; Schwarz, G.; Tsujimoto, M.; Barlow, M.; Wesson, R.; Bode, M.; Corradi, R.; Rodriguez-Gil, P.; Drew, J.; Gaensicke, B.; Steeghs, Daniel; Knigge, C.; Takai, D.; Zijlstra, A.
Bibliographical reference

The Astronomer's Telegram, #1603

Advertised on:
7
2008
Number of authors
19
IAC number of authors
0
Citations
5
Refereed citations
3
Description
We report a new observation of Nova Vul 2007 (S. Nakano, IAUC 8861) obtained by the Swift X-ray Telescope (XRT) on 2008 June 18. The nova was detected at count rate of 0.023 count/s, representing a decline by a factor of 3 compared with Swift XRT observations obtained during 2007 November- December, and by about 50% compared with the previous observation obtained on 2007 December 27. The XRT spectrum is significantly softer than during the earlier epoch, with a ratio of X-ray counts in the 1-10 keV band to those in the 0.3-1 keV band having declined from about 1.0 to 0.4.