XMM-Newton observations ofβCentauri (B1 III): The temperature structure in the hot plasma and the photosphere-wind connection-Reference-Cited by-同舟云学术

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XMM-Newton observations ofβCentauri (B1 III): The temperature structure in the hot plasma and the photosphere-wind connection

Published:2005-06-21 Issue:2 Volume:437 Page:599-609
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Raassen A. J. J.,Cassinelli J. P.,Miller N. A.,Mewe R.,Tepedelenlioǧlu E.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20052650/pdf

Reference53 articles.

1. An X-ray survey of beta Cephei stars

2. Abundances of the elements: Meteoritic and solar

3. A study of coronal abundances in RS CVn binaries

4. β Centauri: An eccentric binary with twoβ Cep-type components

5. Ratio of Line Intensities in Helium-Like Ions as a Density Indicator.

Cited by 15 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A multiwavelength study of SXP 1062, the long-period X-ray pulsar associated with a supernova remnant;Monthly Notices of the Royal Astronomical Society;2017-12-06

2. B stars seen at high resolution by XMM-Newton;Astronomy & Astrophysics;2017-12

3. The pulsating magnetosphere of the extremely slowly rotating magnetic β Cep star ξ1 CMa;Monthly Notices of the Royal Astronomical Society;2017-07-01

4. X-ray diagnostics of massive star winds;Advances in Space Research;2016-09

5. Massive pulsating stars observed by BRITE-Constellation;Astronomy & Astrophysics;2016-03-17

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