A VLBI polarization study of SiO masers towards VY CMa

L. L. Richter; A. J. Kemball; J. L. Jonas

doi:10.1017/S1743921307013269

A VLBI polarization study of SiO masers towards VY CMa

L. L. Richter, A. J. Kemball, J. L. Jonas

Research output: Contribution to journal › Article › peer-review

Abstract

Maser emission from the SiO molecule has been widely observed in the near-circumstellar envelopes of late-type, evolved stars. VLBI images can resolve individual SiO maser spots, providing information about the kinematics and magnetic field in the extended atmospheres of these stars. This poster presents full polarization images of several SiO maser lines towards the supergiant star VY CMa. VY CMa is a particularly strong SiO maser source and allows observations of a wide range of maser transitions. We discuss implications of these observations for VY CMa morphology, polarization, and pumping models.

Original language	English (US)
Pages (from-to)	328-329
Number of pages	2
Journal	Proceedings of the International Astronomical Union
Volume	3
Issue number	S242
DOIs	https://doi.org/10.1017/S1743921307013269
State	Published - Mar 2007

Keywords

Polarization
Stars: late-type

ASJC Scopus subject areas

Medicine (miscellaneous)
Astronomy and Astrophysics
Nutrition and Dietetics
Public Health, Environmental and Occupational Health
Space and Planetary Science

Online availability

10.1017/S1743921307013269

Library availability

Discover UIUC Full Text

Cite this

@article{c4f4f5ab9fa44c23825f31d60f1ebd86,

title = "A VLBI polarization study of SiO masers towards VY CMa",

abstract = "Maser emission from the SiO molecule has been widely observed in the near-circumstellar envelopes of late-type, evolved stars. VLBI images can resolve individual SiO maser spots, providing information about the kinematics and magnetic field in the extended atmospheres of these stars. This poster presents full polarization images of several SiO maser lines towards the supergiant star VY CMa. VY CMa is a particularly strong SiO maser source and allows observations of a wide range of maser transitions. We discuss implications of these observations for VY CMa morphology, polarization, and pumping models.",

keywords = "Polarization, Stars: late-type",

author = "Richter, {L. L.} and Kemball, {A. J.} and Jonas, {J. L.}",

note = "Funding Information: I gratefully acknowledge the support of the NRF, the Fuchs Foundation and the Rhodes University Physics Department.",

year = "2007",

month = mar,

doi = "10.1017/S1743921307013269",

language = "English (US)",

volume = "3",

pages = "328--329",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

number = "S242",

}

TY - JOUR

T1 - A VLBI polarization study of SiO masers towards VY CMa

AU - Richter, L. L.

AU - Kemball, A. J.

AU - Jonas, J. L.

N1 - Funding Information: I gratefully acknowledge the support of the NRF, the Fuchs Foundation and the Rhodes University Physics Department.

PY - 2007/3

Y1 - 2007/3

N2 - Maser emission from the SiO molecule has been widely observed in the near-circumstellar envelopes of late-type, evolved stars. VLBI images can resolve individual SiO maser spots, providing information about the kinematics and magnetic field in the extended atmospheres of these stars. This poster presents full polarization images of several SiO maser lines towards the supergiant star VY CMa. VY CMa is a particularly strong SiO maser source and allows observations of a wide range of maser transitions. We discuss implications of these observations for VY CMa morphology, polarization, and pumping models.

AB - Maser emission from the SiO molecule has been widely observed in the near-circumstellar envelopes of late-type, evolved stars. VLBI images can resolve individual SiO maser spots, providing information about the kinematics and magnetic field in the extended atmospheres of these stars. This poster presents full polarization images of several SiO maser lines towards the supergiant star VY CMa. VY CMa is a particularly strong SiO maser source and allows observations of a wide range of maser transitions. We discuss implications of these observations for VY CMa morphology, polarization, and pumping models.

KW - Polarization

KW - Stars: late-type

UR - http://www.scopus.com/inward/record.url?scp=38849209896&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=38849209896&partnerID=8YFLogxK

U2 - 10.1017/S1743921307013269

DO - 10.1017/S1743921307013269

M3 - Article

AN - SCOPUS:38849209896

VL - 3

SP - 328

EP - 329

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - S242

ER -

A VLBI polarization study of SiO masers towards VY CMa

Abstract

Keywords

ASJC Scopus subject areas

Online availability

Library availability

Related links

Fingerprint

Cite this