Variability of emission lines in the planetary nebulae IC 4997 and NGC 6572-Reference-Cited by-同舟云学术

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Variability of emission lines in the planetary nebulae IC 4997 and NGC 6572

Published:1992-05 Issue: Volume:104 Page:339
ISSN:0004-6280
Container-title:Publications of the Astronomical Society of the Pacific
language:en
Short-container-title:PASP

Author:

Feibelman Walter A.,Aller Lawrence H.,Hyung Siek

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/1538-3873/104/i=675/a=339/pdf

Cited by 27 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. LAMOST J040901.83+329355.6 – a new Galactic star with Wolf–Rayet characteristics in the transitional stage from post-asymptotic giant branch to central star of a planetary nebula;Monthly Notices of the Royal Astronomical Society;2023-12-23

2. Physical conditions and chemical abundances of the variable planetary nebula IC 4997;Monthly Notices of the Royal Astronomical Society;2022-05-16

3. Abundance discrepancy factors in high-density planetary nebulae;Monthly Notices of the Royal Astronomical Society;2022-01-07

4. An episodically variable stellar wind in the planetary nebula IC 4997;Astronomy & Astrophysics;2022-01

5. The real time evolution of post-AGB stars;Proceedings of the International Astronomical Union;2019-10

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