H2O Maser Outflow from the Red Supergiant Star NML Cygni Observed with Japanese VLBI Network-Reference-Cited by-同舟云学术

H2O Maser Outflow from the Red Supergiant Star NML Cygni Observed with Japanese VLBI Network

Published:2008-10-25 Issue:5 Volume:60 Page:1069-1075
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:Publ Astron Soc Jpn

Author:

Nagayama Takumi,Takeda Koji,Omodaka Toshihiro,Imai Hiroshi,Kameno Seiji,Sofue Yoshiaki,Doi Akihiro,Fujisawa Kenta,Habe Asao,Honma Mareki,Kawaguchi Noriyuki,Kawai Eiji,Kobayashi Hideyuki,Koyama Yasuhiro,Murata Yasuhiro,Sorai Kazuo,Sudou Hiroshi,Takaba Hiroshi,Tamura Sayaka,Wakamatsu Ken-Ichi

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/60/5/1069/17453265/pasj60-1069.pdf

Reference30 articles.

1. Sub-au imaging of water vapour clouds around four asymptotic giant branch stars

2. Bispectrum speckle interferometry observations and radiative transfer modelling of the red supergiant NML Cyg

3. Kinematics of the H2O Masers in W49N: Analysis of the Velocity Variance‐Covariance Matrix

4. Ground‐State SiO Maser Emission toward Evolved Stars

5. Rotation in the Envelope of an Evolved Star: Observations of the S[CLC]i[/CLC]O Masers Toward NML Cygni

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