The Be/X-ray transient 4U 0115+63/V635 Cassiopeiae III. Quasi-cyclic variability

Astronomy and Astrophysics

Volumn 462, Issue 3, 2007, Pages 1081-1089

  Reig, P ^a,b   Larionov, V ^c   Negueruela, I ^d   Arkharov, A A ^e   Kudryavtseva, N A ^c,f  

^a INSTITUTE OF ELECTRONIC STRUCTURE AND LASER   (Greece)

^b UNIVERSITY OF CRETE   (Greece)

^c ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

^d UNIVERSITY OF ALICANTE   (Spain)

^e RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^f MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

Author keywords

Stars: binaries: close; Stars: emission line, Be; Stars: neutron; Stars: pulsars: individual: 4U 0115+63; Stars: pulsars: individual: V635 Cas; X rays: binaries

Indexed keywords

GALAXIES; INFRARED RADIATION; LIGHT EMISSION; OPTICAL CORRELATION; PERTURBATION TECHNIQUES; SPECTROSCOPIC ANALYSIS; X RAYS;

NEUTRON STARS; PULSARS; X-RAY OUTBURSTS;

ASTROPHYSICS;

EID: 33846798120     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066217     Document Type: Article

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