Variability of hot supergiant IRAS 19336-0400 in the early phase of planetary nebula ionization-Reference-Cited by-同舟云学术

Variability of hot supergiant IRAS 19336-0400 in the early phase of planetary nebula ionization

Published:2012-03 Issue:3 Volume:38 Page:157-166
ISSN:1063-7737
Container-title:Astronomy Letters
language:en
Short-container-title:Astron. Lett.

Author:

Arkhipova V. P.,Burlak M. A.,Esipov V. F.,Ikonnikova N. P.,Komissarova G. V.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1134/S1063773712020016.pdf

Reference27 articles.

1. G. A. Alekseeva, A. A. Arkharov, V. D. Galkin, et al., VizieR Online Data Catalog III/201 (1997).

2. V. P. Arkhipova, N. P. Ikonnikova, G. V. Komissarova, and R. I. Noskova, Planetary Nebulae in our Galaxy and Beyond, IAU Symp. 234. (Ed. Ian F. Corbett, Cambridge: Cambridge Univ. Press, 2006), pp. 357–358.

3. A. A. Boyarchuk and I. I. Pronik, Izv. Krym. Astrofiz. Obs. 33, 195 (1965).

4. J. D. Bregman, D. Jesse, D. Rank, et al., Astrophys. J. 411, 794 (1993).

5. L. Cerrigone, J. L. Hora, G. Umana, and C. Trigilio, Astrophys. J. 703, 585 (2009).

Cited by 6 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. Analysis of absorption lines in the high-resolution spectra of five hot post-AGB candidates;Monthly Notices of the Royal Astronomical Society;2020-03-28

2. High-resolution spectroscopy of the high-velocity hot post-AGB star IRAS 18379–1707 (LS 5112);Monthly Notices of the Royal Astronomical Society;2019-11-29

3. Line identification and photometric history of the hot post-AGB star Hen 3−1013 (IRAS 14331−6435);Monthly Notices of the Royal Astronomical Society;2018-09-10

4. Imaging the transition between pre-planetary and planetary nebulae: integral field spectroscopy of hot post-AGB stars with NIFS;Monthly Notices of the Royal Astronomical Society;2014-12-19

5. Variability and possible rapid evolution of the hot post-AGB stars Hen 3-1347, Hen 3-1428, and LSS 4634;Astronomy Letters;2014-08