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Cited article:

X-ray and UV observations of nova V598 Puppis between 147 and 255 days after outburst

K. L. Page, J. P. Osborne, A. M. Read, P. A. Evans, J.-U. Ness, A. P. Beardmore, M. Bode, G. J. Schwarz, S. Starrfield

A&A, 507 2 (2009) 923-927

Published online: 2009-09-15

DOI: https://doi.org/10.1051/0004-6361/200912985

This article has been cited by the following article(s):

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Do novae have optically thick winds during outburst with large deviations from spherical symmetry?

M. Friedjung
Astronomy & Astrophysics 536 A97 (2011)
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SWIFT X-RAY OBSERVATIONS OF CLASSICAL NOVAE. II. THE SUPER SOFT SOURCE SAMPLE

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The Astrophysical Journal Supplement Series 197 (2) 31 (2011)
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X-Ray Study of Rekindled Accretion in the Classical Nova V2491 Cygni

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Publications of the Astronomical Society of Japan 63 (sp3) S729 (2011)
https://doi.org/10.1093/pasj/63.sp3.S729

The XMM-Newton detection of extended emission from the nova remnant of T Pyxidis

Ş. Balman
Monthly Notices of the Royal Astronomical Society: Letters 404 (1) L26 (2010)
https://doi.org/10.1111/j.1745-3933.2010.00827.x