Formation of Complex Organic Molecules (COMs) from Polycyclic Aromatic Hydrocarbons (PAHs): Implications for ISM IR Emission Plateaus and Solar System Organics-Reference-Cited by-同舟云学术

Formation of Complex Organic Molecules (COMs) from Polycyclic Aromatic Hydrocarbons (PAHs): Implications for ISM IR Emission Plateaus and Solar System Organics

Published:2020-11-20 Issue:12 Volume:4 Page:2227-2245
ISSN:2472-3452
Container-title:ACS Earth and Space Chemistry
language:en
Short-container-title:ACS Earth Space Chem.

Author:

Mattioda Andrew L.¹^ORCID,Cruz-Diaz Gustavo A.¹²,Ging Andrew¹,Barnhardt Michael¹,Boersma Christiaan¹³,Allamandola Louis J.¹²,Schneider Todd⁴,Vaughn Jason⁴,Phillips Brandon⁴,Ricca Alessandra¹⁵

Affiliation:

1. NASA Ames Research Center, MS 245-6, Moffett Field, California 94035, United States

2. Bay Area Environmental Research Institute, P.O. Box 25, Moffett Field, California 94035, United States

3. San Jose State University Research Foundation, 210 North 4th Street, San Jose, California 95112, United States

4. NASA Marshall Space Flight Center, Huntsville, Alabama 35824, United States

5. SETI Institute, 189 Bernardo Avenue, Suite 200, Mountain View, California 94043, United States

Funder

Astrophysics Science Division

National Aeronautics and Space Administration

Publisher

American Chemical Society (ACS)

Subject

Space and Planetary Science,Atmospheric Science,Geochemistry and Petrology

Link

https://pubs.acs.org/doi/pdf/10.1021/acsearthspacechem.0c00165

Reference69 articles.

1. The Organic Refractory Material in the Diffuse Interstellar Medium: Mid‐Infrared Spectroscopic Constraints

2. Pendleton, Y. In Hydrocarbons in Meteorites, the Milky Way, and Other Galaxies, Astrophysics of Dust, ASP Conference Series, 2003; p 573.

3. The PAH Hypothesis

4. Stability of Condensed Hydrocarbons in the Solar Nebula

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