Variability of the planetary nebula NGC 6572 and its central star during the interval covered by optical observations-Reference-Cited by-同舟云学术

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Variability of the planetary nebula NGC 6572 and its central star during the interval covered by optical observations

Published:2014-10 Issue:10 Volume:58 Page:702-715
ISSN:1063-7729
Container-title:Astronomy Reports
language:en
Short-container-title:Astron. Rep.

Author:

Arkhipova V. P.,Kostyakova E. B.,Burlak M. A.,Esipov V. F.,Ikonnikova N. P.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1134/S1063772914100023.pdf

Reference66 articles.

1. L. Aller and W. Liller, Mon. Not. R. Astron. Soc. 132, 337 (1966).

2. B. A. Vorontsov-Vel’yaminov, Sov. Astron. 5, 186 (1961).

3. L. Kohoutek, Bull. Astron. Inst. Czechosl. 17, 318 (1966).

4. R. Tylenda, A. Acker, and B. Stenholm, Astron. Astrophys. Suppl. Ser. 102, 595 (1993).

5. L. Kohoutek, Catalogue of Galactic Planetary Nebulae (Hamburger Sternwarte, Hamburg-Bergedorf, 2001), p. 31.

Cited by 2 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. Morpho-kinematic and photoionization models of the multipolar structures in planetary nebula NGC 6572;Monthly Notices of the Royal Astronomical Society;2023-06-22

2. A search for photometric and spectroscopic evolutionary changes in the young planetary nebula Vy 2-2;Astronomy Letters;2017-12

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