TheXMM-Newtondetection of extended emission from the nova remnant of T Pyxidis
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/404/1/L26/3183259/404-1-L26.pdf
Reference48 articles.
1. ChandraObservation of the Shell of Nova Persei 1901 (GK Persei): Detection of Localized Nonthermal X‐Ray Emission from a Miniature Supernova Remnant
2. An archival study of extended X-ray emission from classical and recurrent novae
3. The First Resolved and Detected Classical Nova Shell in X-Rays: The Shell of Nova Persei 1901
4. The X‐Ray Spectral Evolution of Classical Nova V1974 Cygni 1992: A Reanalysis of theROSATData
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1. The Long-term Secular Mass Accretion Rate of the Recurrent Nova T Pyxidis;The Astrophysical Journal;2018-07-25
2. Pre-outburstChandraobservations of the recurrent nova T Pyxidis;Astronomy & Astrophysics;2014-12
3. THE 2011 OUTBURST OF RECURRENT NOVA T Pyx: X-RAY OBSERVATIONS EXPOSE THE WHITE DWARF MASS AND EJECTION DYNAMICS;The Astrophysical Journal;2014-05-30
4. THE 2011 ERUPTION OF THE RECURRENT NOVA T PYXIDIS: THE DISCOVERY, THE PRE-ERUPTION RISE, THE PRE-ERUPTION ORBITAL PERIOD, AND THE REASON FOR THE LONG DELAY;The Astrophysical Journal;2013-07-25
5. DYNAMICAL FRAGMENTATION OF THE T PYXIDIS NOVA SHELL DURING RECURRENT ERUPTIONS;The Astrophysical Journal;2013-04-12
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