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27 April 2024 |
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The Be/X-ray binary system V 0332+53: A Short Review | | M. D. Caballero-Garcia
; A. Camero-Arranz
; M. Ozbey Arabaci
; R. Hudec
; on behalf of a larger collaboration
; | | Date: |
1 Sep 2015 | | Abstract: | Be/X-ray binary systems provide an excellent opportunity to study the physics
around neutron stars through the study of the behaviour of matter around them.
Intermediate and low-luminosity type outbursts are interesting because they
provide relatively clean environments around neutron stars. In these conditions
the physics of the magnetosphere around the neutron star can be better studied
without being very disturbed by other phenomena regarding the transfer of
matter between the two components of the Be/X-ray binary system. A recent study
presents the optical longterm evolution of the Be/X-ray binary V 0332+53 plus
the X-ray emission mainly during the intermediate-luminosity outburst on 2008.
In this paper we comment on the context of these observations and on the
properties that can be derived through the analysis of them. | | Source: | arXiv, 1509.0230 | | Services: | Forum | Review | PDF | Favorites | |
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