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

Monthly Notices of the Royal Astronomical Society: Letters

Volumn 404, Issue 1, 2010, Pages

  Balman, S ^a,b  

^a MIDDLE EAST TECHNICAL UNIVERSITY   (Turkey)

^b UNIVERSITY OF WARWICK   (United Kingdom)

Author keywords

Binaries: close; Novae, cataclysmic variables; Radiation mechanisms: thermal; Shock waves; Stars: individual: T pyxidis; X rays: stars

Indexed keywords

EID: 79952477210     PISSN: 17453933     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1745-3933.2010.00827.x     Document Type: Letter

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