Hostname: page-component-78c5997874-94fs2 Total loading time: 0 Render date: 2024-11-17T14:50:38.179Z Has data issue: false hasContentIssue false
  • English
  • Français

Swift Observations of Novae

Published online by Cambridge University Press:  17 January 2013

K. L. Page
K. L. Page*
Affiliation:
Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The rapid response capability of Swift, together with the daily planning of its observing schedule, make it an ideal mission for following novae in the X-ray and UV bands. A number of both classical and recurrent novae have been extensively monitored throughout their supersoft phase. We report findings from these observations, including the high-amplitude flux variation often seen at the start of the supersoft emission, the optical plateau sometimes seen for recurrent novae, the differing relationships between the X-ray and UV variability, and the turn-on and turn-off times of the supersoft emission for the Swift sample of novae.

Keywords

novaecataclysmic variables
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Issue S281: Binary Paths to Type Ia Supernovae Explosions , July 2011 , pp. 96 - 104
Copyright
Copyright © International Astronomical Union 2013

References

Beardmore, A. P.et al. 2010, ATel, 2423Google Scholar
Beardmore, A. P., Osborne, J. P., Page, K., Schwarz, G. J., Starrfield, S., & Ness, J.-U. 2008, ATel, 1873Google Scholar
Burrows, D. N.et al. 2005, Space Science Review, 120, 165CrossRefGoogle Scholar
Drake, J. J.et al. 2008, ATel, 1721Google Scholar
Drake, J. J.et al. 2003, ApJ, 584, 448Google Scholar
Evans, A., Bode, M. F., O'Brien, T. J. and Darnley, M. J. (eds.), RS Ophiuchi (2006) and the Recurrent Nova Phenomenon, ASP Conference Series 401Google Scholar
Gehrels, N.et al. 2004, ApJ, 611, 1005Google Scholar
Greiner, J., Orio, M., & Schartel, N. 2003, A&A, 405, 703Google Scholar
Hachisu, I. & Kato, M. 2010, ApJ, 709, 680Google Scholar
Hachisu, I.et al. 2008, in: Evans, A., Bode, M. F., O'Brien, T. J. and Darnley, M. J. (eds.), RS Ophiuchi (2006) and the Recurrent Nova Phenomenon, ASP Conference Series 401, 206Google Scholar
Krautter, J., Ögelman, H., Starrfield, S., Wichmann, R., & Pfeffermann, E. 2005, ApJ, 456, 788Google Scholar
Osborne, J. P.et al. 2011, ApJ, 727, 124CrossRefGoogle Scholar
Ness, J.-U.et al. 2009, AJ, 137, 4160CrossRefGoogle Scholar
Ness, J.-U.et al. 2007, ApJ, 665, 1334Google Scholar
Ness, J.-U.et al. 2003, ApJ, 594, L127Google Scholar
Page, K. L.et al. 2010, MNRAS, 401, 121Google Scholar
Orio, M., Parmar, A. N., Greiner, J., Ögelman, H., Starrfield, S., & Trussoni, E. 2002, MNRAS, 333, L11Google Scholar
Roming, P. W. A.et al. 2005, Space Science Review, 120, 95CrossRefGoogle Scholar
Schwarz, G. J.et al. 2011, ApJ, submittedGoogle Scholar
Shore, S. N. 2008, in: Bode, M. & Evans, A. (eds.), Classical Novae 2nd Edition (Cambridge University Press), p. 194Google Scholar