Phenomenological model of the antiflare star RZ Psc-Reference-Cited by-同舟云学术

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Phenomenological model of the antiflare star RZ Psc

Published:1981 Issue:1 Volume:17 Page:47-52
ISSN:0571-7132
Container-title:Astrophysics
language:en
Short-container-title:Astrophysics

Author:

Pugach A. F.

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF01014295.pdf

Reference17 articles.

1. L. V. Mirzoyan, in: Early Stages in the Evolution of Stars [in Russian], Naukova Dumka, Kiev (1977), p. 100.

2. G. V. Zaitseva, Peremennye Zvezdy,16, 435 (1968).

3. G. V. Zaitseva, V. M. Lyutyi, and A. M. Cherepashuk, Astrofizika,10, 357 (1974).

4. W. Wenzel, in: Non-Periodic Phenomena in Variable Stars, IAU Colloq., Budapest (1969). p. 61.

5. W. Wenzel, MVS,5, 75 (1970).

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1. Magnetospheric accretion at the late phases of the pre-main-sequence evolution: the case of RZ Psc;Monthly Notices of the Royal Astronomical Society;2023-02-02

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3. Radial Velocity Fluctuations of RZ Psc;Astrophysics;2014-11-18

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