Long-term optical and X-ray variability of the Be/X-ray binary H 1145-619: Discovery of an ongoing retrograde density wave

Journal Article

2017

Permanent link to this Item
http://hdl.handle.net/11427/34212
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AlfonsoGarznJ_Long_term_optic_2017.pdf (1.75 MB)
Authors
Alfonso-Garzón, J
Fabregat, J
Reig, P
Kajava, J J E
Sánchez-Fernández, C
Townsend, L J
Mas-Hesse, J M
Crawford, S M
Kretschmar, P
Coe, M J
Journal Title

Astronomy and Astrophysics

Link to Journal
https://dx.doi.org/10.1051/0004-6361/201630211
Journal ISSN
Volume Title
Publisher
Publisher
Department
Department of Astronomy
Faculty
Faculty of Science
License
Series
Abstract
Context. Multiwavelength monitoring of Be/X-ray binaries is crucial to understand the mechanisms producing their outbursts. H 1145-619 is one of these systems, which has recently displayed X-ray activity.
Description
Keywords
X-rays: binaries
stars: emission-line, Be
stars: neutron
techniques: photometric
techniques: spectroscopic
stars: emission-line
Be

Reference:

Alfonso-Garzón, J., Fabregat, J., Reig, P., Kajava, J.J.E., Sánchez-Fernández, C., Townsend, L.J., Mas-Hesse, J.M. & Crawford, S.M. et al. 2017. Long-term optical and X-ray variability of the Be/X-ray binary H 1145-619: Discovery of an ongoing retrograde density wave. Astronomy and Astrophysics. 607(4):A52 - 177. http://hdl.handle.net/11427/34212

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