A MOST probable explanation of the pulsation of WR 123-Reference-Cited by-同舟云学术

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A MOST probable explanation of the pulsation of WR 123

Published:2006-06-28 Issue:3 Volume:453 Page:L35-L37
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Dorfi E. A.,Gautschy A.,Saio H.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:200600027/pdf

Reference18 articles.

1. Wolf-Rayet Stars

2. Dorfi, E. A. 1998, 27th Saas Fee Course (Berlin: Springer), 263

3. Where Are the Regularly Pulsating Massive Stars?

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1. A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars. III. The northern late-type nitrogen-rich sample;Astronomy & Astrophysics;2022-12-05

2. Multiple variability time-scales of the early nitrogen-rich Wolf–Rayet star WR 7;Monthly Notices of the Royal Astronomical Society;2022-05-30

3. Red noise and pulsations in evolved massive stars;Monthly Notices of the Royal Astronomical Society;2021-01-16

4. The Galactic WN stars revisited;Astronomy & Astrophysics;2019-05

5. References;Pulsating Stars;2015-08-21

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