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Cited article:

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Multiwavelength observations of V407 Lupi (ASASSN-16kt) – a very fast nova erupting in an intermediate polar

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The slow decline of the Galactic recurrent novae T Pyxidis, IM Normae, and CI Aquilae

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X-ray monitoring of classical novae in the central region of M 31 III. Autumn and winter 2009/10, 2010/11, and 2011/12

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THE 7.1 HR X-RAY-ULTRAVIOLET-NEAR-INFRARED PERIOD OF THE γ-RAY CLASSICAL NOVA MONOCEROTIS 2012

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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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Novae as a Class of Transient X‐Ray Sources

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V5116 Sagittarii, an Eclipsing Supersoft Postoutburst Nova?

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V723 CASSIOPEIA STILL ON IN X-RAYS: A BRIGHT SUPER SOFT SOURCE 12 YEARS AFTER OUTBURST

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SwiftX‐Ray Observations of Classical Novae

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An X-ray-emitting blast wave from the recurrent nova RS Ophiuchi

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Supersoft X‐Ray Sources in M31. II.ROSAT‐detected Supersoft Sources in theROSAT,Chandra, andXMM‐NewtonEras

J. Greiner, R. Di Stefano, A. Kong and F. Primini
The Astrophysical Journal 610 (1) 261 (2004)
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