The importance of soft X-rays for the excitation of H2 emission in planetary nebulae
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/368/2/819/3080893/mnras0368-0819.pdf
Reference56 articles.
1. Detection of molecular hydrogen emission from five planetary nebulae
2. Interstellar H2 - The population of excited rotational states and the infrared response to ultraviolet radiation
3. Fluorescent excitation of interstellar H2
Cited by 8 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. Extended Structures of Planetary Nebulae Detected in H2 Emission;The Astrophysical Journal;2018-05-29
2. H2in low-ionization structures of planetary nebulae;Monthly Notices of the Royal Astronomical Society;2016-12-08
3. Spitzermid-infrared spectroscopic observations of planetary nebulae;Monthly Notices of the Royal Astronomical Society;2016-03-17
4. HerschelPlanetary Nebula Survey (HerPlaNS);Astronomy & Astrophysics;2014-06
5. H2infrared line emission from the ionized region of planetary nebulae;Astronomy & Astrophysics;2011-03-03
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