The X-ray emission from Nova V382 Velorum - I. the hard component observed with BeppoSAX

Monthly Notices of the Royal Astronomical Society

Volumn 326, Issue 2, 2001, Pages L13-L18

  Orio, M ^a,b   Parmar, A ^c   Benjamin, R ^d   Amati, L ^e   Frontera, F ^e   Greiner, J ^f   Ogelman H ^d   Mineo, T ^e   Starrfield, S ^g   Trussoni, E ^a  

^a OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

^b UNIVERSITY OF WISCONSIN MADISON   (United States)

^c EUROPEAN SPACE AGENCY   (Netherlands)

^d University of Wisconsin Madison   (United States)

^e CNR   (Italy)

^f ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^g ARIZONA STATE UNIVERSITY   (United States)

Author keywords

Novae, cataclysmic variables; Stars: individual: V382 Vel; X rays: stars

Indexed keywords

ELECTRON TEMPERATURE;

HARD COMPONENTS; NOVAE CATACLYSMIC VARIABLES; PLASMA TEMPERATURE; STAR: INDIVIDUAL: V382 VEL; STARS: INDIVIDUAL: PROXIMA CENTAURI; UPPER LIMITS; X RAY BANDS; X-RAY EMISSION; X-RAY SOURCES; X-RAY:STARS;

STARS;

EID: 18044402722     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04448.x     Document Type: Article

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