Time-resolved high-resolution spectroscopy of CH Cygni: evidence for a magnetic propeller state in 1994-Reference-Cited by-同舟云学术

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Time-resolved high-resolution spectroscopy of CH Cygni: evidence for a magnetic propeller state in 1994

Published:1996-01-11 Issue:2 Volume:278 Page:542-550
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Tomov T.,Kolev D.,Munari U.,Antov A.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/278/2/542/2793464/278-2-542.pdf

Cited by 19 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. High-velocity equatorial mass ejections and some other spectroscopic phenomena of the symbiotic star CH Cygni in an active stage;Astronomy & Astrophysics;2019-01-24

2. Active Stage of the Object CH Cyg B in 2014-2015;Astrophysics;2017-06

3. SimultaneousUBVRIobservations of the cataclysmic variable AE Aquarii: Temperatures and masses of fireballs;Astronomische Nachrichten;2012-10

4. CH Cygni in 2004 – II: Nebular spectrum features;New Astronomy;2007-10

5. The high resolution spectra of symbiotic star CH Cygni in 2004;New Astronomy;2006-03

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