Magnetically aligned dust and SiO maser polarisation in the envelope of the red supergiant VY Canis Majoris-Reference-Cited by-同舟云学术

Magnetically aligned dust and SiO maser polarisation in the envelope of the red supergiant VY Canis Majoris

Published:2017-07 Issue: Volume:603 Page:A92
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Vlemmings W. H. T.^ORCID,Khouri T.,Martí-Vidal I.,Tafoya D.,Baudry A.,Etoka S.,Humphreys E. M. L.,Jones T. J.,Kemball A.,O’Gorman E.,Pérez-Sánchez A. F.,Richards A. M. S.

Funder

European Research Council

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201730735/pdf

Reference47 articles.

1. Interstellar Dust Grain Alignment

2. INTERFEROMETRIC MAPPING OF MAGNETIC FIELDS: THE ALMA VIEW OF THE MASSIVE STAR-FORMING CLUMP W43-MM1

3. Characteristics of dust shells around 13 late-type stars

4. The Polarization of Starlight by Aligned Dust Grains.

5. ALMA observations of TiO2around VY Canis Majoris

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