The structure of the planetary nebula NGC 2371 in the visible and mid-infrared-Reference-Cited by-同舟云学术

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The structure of the planetary nebula NGC 2371 in the visible and mid-infrared

Published:2012-08-13 Issue:2 Volume:425 Page:1091-1103
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:

Ramos-Larios Gerardo¹,Phillips J. P.¹

Affiliation:

1. Instituto de Astronomía y Meteorología; Av. Vallarta No. 2602, Col. Arcos Vallarta, C.P.; 44130; Guadalajara; Jalisco; Mexico

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/425/2/1091/4015067/425-2-1091.pdf

Reference65 articles.

1. A spectroscopic study of moderately bright planetary nebulae

2. NGC 6543. I. Understanding the Anatomy of the Cat's Eye

3. FLIERs and other microstructures in planetary nebulae, 2

Cited by 4 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. Planetary nebulae with Wolf–Rayet-type central stars – I. The case of the high-excitation NGC 2371;Monthly Notices of the Royal Astronomical Society;2020-06-03

2. Planetary Nebulae that Cannot Be Explained by Binary Systems;The Astrophysical Journal;2017-03-02

3. Ionization structure of multiple-shell planetary nebulae;Astronomy & Astrophysics;2014-05

4. A revised distance scale of planetary nebulae;Astronomy & Astrophysics;2013-12

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