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XMM-Newton and Swift Observations of WZ Sagittae: Spectral and Timing AnalysisWZ Sagittae is the prototype object of a subclass of dwarf novae with rare and long (super)outbursts, in which a white dwarf primary accretes matter from a low mass companion. High-energy observations offer the possibility of a better understanding of the disk-accretion mechanism in WZ Sge-like binaries.
Document ID
20150023319
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1051/0004-6361/201322875
Authors
Nucita, A. A. (Universita del Salento Lecce LE, Italy)
Kuulkers, E. (European Space Astronomy Centre (ESAC) Madrid, Spain)
De Paolis, F. (Universita del Salento Lecce LE, Italy)
Mukai, K. (Maryland Univ. Baltimore, MD, United States)
Ingrosso, G. (Universita del Salento Lecce LE, Italy)
Maiolo, B. M. T. (Universita del Salento Lecce LE, Italy)
Date Acquired
December 18, 2015
Publication Date
June 23, 2014
Publication Information
Publication: Astonomy & Astrophysics Worlwide Atronomical and Astrophysical Research
Publisher: EDP Sciences
Volume: 566
Subject Category
Astrophysics
Astronomy
Report/Patent Number
GSFC-E-DAA-TN24188
Funding Number(s)
CONTRACT_GRANT: NNG06EO9A
Distribution Limits
Public
Copyright
Other
Keywords
binaries: general aEuro" white dwarfs aEuro" X-rays: binaries

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