Spectral imaging of the Orion Bar at 3.3, 8.4, and 11.3 microns: Comparison with a fluorescent polycyclic aromatic hydrocarbon model
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 21 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. Rank, David M.;Biographical Encyclopedia of Astronomers;2022
2. Orion Bar as a window to the evolution of PAHs;Monthly Notices of the Royal Astronomical Society;2021-10-22
3. Experimental and theoretical studies of photoinduced reactions in the solid phase of the interstellar medium;Russian Chemical Reviews;2020-04-01
4. 3.3μm PAH observations of the central kiloparsecs of Centaurus A;Astronomy & Astrophysics;2013-03
5. TEARING THE VEIL: INTERACTION OF THE ORION NEBULA WITH ITS NEUTRAL ENVIRONMENT;The Astrophysical Journal;2012-12-20
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