M. D. Caballero-Garcia, A. Camero-Arranz, M. Ozbey Arabaci, R. Hudec, on behalf of a larger collaboration
Published 2015-09-01Version 1
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.
Comments: Submitted to PoS (Invited talk in Frascati 2015 conference "XI Multifrequency Behaviour of High Energy Cosmic Sources Workshop"; Palermo, Italy). 5 pages, 2 figures
Activity from the Be/X-ray binary system V0332+53 during its low-luminosity outburst in 2008
Explosive Combustion of a Neutron Star into a Quark Star: the non-premixed scenario
Neutron stars in a perturbative $f(R)$ gravity model with strong magnetic fields
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