AN APPARENT PRECESSING HELICAL OUTFLOW FROM A MASSIVE EVOLVED STAR: EVIDENCE FOR BINARY INTERACTION-Reference-Cited by-同舟云学术

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AN APPARENT PRECESSING HELICAL OUTFLOW FROM A MASSIVE EVOLVED STAR: EVIDENCE FOR BINARY INTERACTION

Published:2016-02-12 Issue:2 Volume:818 Page:117
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Lau R. M.,Hankins M. J.,Herter T. L.,Morris M. R.,Mills E. A. C.,Ressler M. E.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/818/i=2/a=117/pdf

Reference77 articles.

1. MEASUREMENT OF SPIN-ORBIT MISALIGNMENT AND NODAL PRECESSION FOR THE PLANET AROUND PRE-MAIN-SEQUENCE STAR PTFO 8-8695 FROM GRAVITY DARKENING

2. Two extremely luminous WN stars in the Galactic center with circumstellar emission from dust and gas

3. Rotating massive main-sequence stars

4. MIPSGAL: A Survey of the Inner Galactic Plane at 24 and 70 μm

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1. SOFIA/FORCAST Galactic Center Legacy Survey: Overview;The Astrophysical Journal;2020-05-05

2. Origins of X-Ray Line Emissions in Circinus X-1 at Very Low X-Ray Flux;The Astrophysical Journal;2020-03-13

3. Study of the Galactic radio sources in the SCORPIO survey resolved by ATCA at 2.1 GHz;Monthly Notices of the Royal Astronomical Society;2019-10-24

4. SOFIA/FORCAST Observations of the Sgr A-H H ii Regions: Using Dust Emission to Elucidate the Heating Sources;The Astrophysical Journal;2019-05-20

5. The young Be-star binary Circinus X-1;Proceedings of the International Astronomical Union;2018-08

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