Cyclical behaviour and disc truncation in the Be/X-ray binary A0535+26
- Autor
- HAIGH, N. J1 ; COE, M. J1 ; FABREGAT, J2
[1] School of Physics and Astronomy, The University, Southampton, SO17 1BJ, United Kingdom
[2] Observatorio Astronómico, Universidad de Valencia, 46100 Burjassot, Spain - Fuente
Monthly Notices of the Royal Astronomical Society. 2004, Vol 350, Num 4, pp 1457-1466, 10 p ; ref : 44 ref
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Campo Científico
- Astronomy earth cosmic environment
- Editor
- Blackwell Science, Oxford
- País de la publicación
- United Kingdom
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave de autor
- X-rays: binaries pulsars stars: emission-line, Be stars: neutron
- Palabra clave (fr)
- Binaire RX Disque accrétion Etat transition Etoile Be Etoile neutron Etoile raie émission Excès IR Masse stellaire Précession Pulsar Source RX binaire Source RX cosmique
- Palabra clave (in)
- X-ray binary stars Accretion disks Transition state Be stars Neutron stars Emission line stars Infrared excess Stellar mass Precession Pulsars Binary X ray source Cosmic x-ray sources
- Palabra clave (es)
- Estado transitorio Exceso IR Fuente RX binaria
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03A Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations / 001E03A10 Fundamental astronomy / 001E03A10G Eclipses, transits, and occultations
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C80 Binary and multiple stars / 001E03C80J X-ray binaries
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 15773330
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1111/j.1365-2966.2004.07743.x 
https://dx.doi.org/10.1111/j.1365-2966.2004.07743.x
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