PAHs and star formation in the H ii regions of nearby galaxies M83 and M33
Author:
Affiliation:
1. Department of Physics and Astronomy, University of Western Ontario, London ON N6A 3K7, Canada
2. SETI Institute, 189 Bernardo Avenue, Suite 100, Mountain View, CA 94043, USA
3. Leiden Observatory, Leiden, the Netherlands
Funder
National Aeronautics and Space Administration
Natural Sciences and Engineering Research Council of Canada
Netherlands Organisation for Scientific Research
Horizon 2020
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/481/4/5370/26038900/sty2658.pdf
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3. The Infrared Spectra of Very Large, Compact, Highly Symmetric, Polycyclic Aromatic Hydrocarbons (PAHs)
4. THE INFRARED SPECTRA OF VERY LARGE IRREGULAR POLYCYCLIC AROMATIC HYDROCARBONS (PAHs): OBSERVATIONAL PROBES OF ASTRONOMICAL PAH GEOMETRY, SIZE, AND CHARGE
5. The 15–20 μm PAH emission features: probes of individual PAHs?
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