A magnetic confinement versus rotation classification of massive-star magnetospheres-Reference-Cited by-同舟云学术

A magnetic confinement versus rotation classification of massive-star magnetospheres

Published:2012-12-03 Issue:1 Volume:429 Page:398-422
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Petit V.,Owocki S. P.,Wade G. A.,Cohen D. H.,Sundqvist J. O.,Gagne M.,Apellaniz J. M.,Oksala M. E.,Bohlender D. A.,Rivinius T.,Henrichs H. F.,Alecian E.,Townsend R. H. D.,ud-Doula A.,Collaboration t. M.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/429/1/398/3353115/sts344.pdf

Reference165 articles.

1. Spectroscopic binaries in the Orion Nebula cluster

2. Characterization of the magnetic field of the Herbig Be star HD 200775★

3. Discovery of magnetic fields in the very young, massive stars W601 (NGC 6611) and OI 201 (NGC 2244)

4. First HARPSpol discoveries of magnetic fields in massive stars

5. High-precision elements of double-lined spectroscopic binaries from combined interferometry and spectroscopy

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