The secrets of T Pyxidis II. A recurrent nova that will not become a SN la

Astronomy and Astrophysics

Volumn 492, Issue 3, 2008, Pages 787-803

  Selvelli, P ^a   Cassatella, A ^b,c   Gilmozzi, R ^d   Gonzalez Riestra R ^e  

^a INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^b INAF   (Italy)

^c ROMA TRE UNIVERSITY   (Italy)

^d EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^e EUROPEAN SPACE AGENCY   (Spain)

Author keywords

Stars: novae, cataclysmic variables; Stars: supernovae: general; Ultraviolet: general; X rays: binaries

Indexed keywords

DISKS (STRUCTURAL COMPONENTS);

ACCRETION RATES; CLASSICAL NOVAE; DECAY TIMES; DIRECT ESTIMATES; LONG DURATIONS; SPECTROSCOPIC BEHAVIORS; STARS: NOVAE, CATACLYSMIC VARIABLES; STARS: SUPERNOVAE: GENERAL; TOTAL MASSES; ULTRAVIOLET: GENERAL; WHITE DWARVES; X-RAYS: BINARIES;

STARS;

EID: 57649231765     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810678     Document Type: Article

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