Fundamental properties of High Mass X-ray Binaries

Fundamental properties of High Mass X-ray Binaries

The aim of this thesis is to characterise a sample of High Mass X-ray Binaries (HMXBs) formed by: IGR J00370+6122, XTE J1855-026, AX J1841.0-0535 and AX J1845.0-0433. These objects are composed of pulsars (rotating neutron stars) accreting material from the wind of their supergiant companions. The X...

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Bibliographic Details
Main Author: González Galán, Ana
Other Authors: Negueruela Díez, Ignacio
Format: Doctoral Thesis
Language:English
Published: Universidad de Alicante 2014
Subjects:
Stars
Binaries
Pulsars
Supergiants
X-rays
Astronomía y Astrofísica
Online Access:http://hdl.handle.net/10045/41723

Internet

http://hdl.handle.net/10045/41723

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