An alternative hypothesis for the outburst mechanism in supergiant fast X-ray transients: The case of IGR J11215-5952

Astronomy and Astrophysics

Volumn 476, Issue 3, 2007, Pages 1307-1315

  Sidoli, L ^a   Romano, P ^b,c   Mereghetti, S ^a   Paizis, A ^a   Vercellone, S ^a   Mangano, V ^d   Gotz D ^e  

^a INAF IASF MILANO   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI BRERA   (Italy)

^c UNIVERSITY OF MILANO BICOCCA   (Italy)

^d INAF IASF PALERMO   (Italy)

^e CEA SACLAY   (France)

Author keywords

Accretion, accretion disks; Stars: neutron; Supergiants; X rays: binaries; X rays: individuals: IGR J11215 5952

Indexed keywords

ORBITS; SPECTRUM ANALYSIS; X RAY ANALYSIS;

BINARY SYSTEMS; ECCENTRIC ORBITS; ORBITAL PERIODS; X-RAY TRANSIENTS;

ASTROPHYSICS;

EID: 38049186657     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078137     Document Type: Article

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