Infrared Spectrum of Protonated Corannulene H+C20H10 in Solid para-Hydrogen and its Potential Contribution to Interstellar Unidentified Infrared Bands-Reference-Cited by-同舟云学术

Infrared Spectrum of Protonated Corannulene H+C20H10 in Solid para-Hydrogen and its Potential Contribution to Interstellar Unidentified Infrared Bands

Published:2018-08-21 Issue:10 Volume:2 Page:1001-1010
ISSN:2472-3452
Container-title:ACS Earth and Space Chemistry
language:en
Short-container-title:ACS Earth Space Chem.

Author:

Sundararajan Pavithraa¹,Tsuge Masashi¹²^ORCID,Baba Masaaki³,Lee Yuan-Pern¹⁴⁵^ORCID

Affiliation:

1. Department of Applied Chemistry and Institute of Molecular Science, National Chiao Tung University, Hsinchu 30010, Taiwan

2. Institute of Low Temperature Science, Hokkaido University, Sapporo 060-0819, Japan

3. Division of Chemistry, Graduate School of Science, Kyoto University, Kyoto 606-8502, Japan

4. Center for Emergent Functional Matter Science, National Chiao Tung University, Hsinchu 30010, Taiwan

5. Institute of Atomic and Molecular Sciences, Academia Sinica, Taipei 10617, Taiwan

Funder

Ministry of Education

Ministry of Education, Culture, Sports, Science and Technology

Ministry of Science and Technology, Taiwan

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.8b00089

Reference42 articles.

1. Interstellar polycyclic aromatic hydrocarbons - The infrared emission bands, the excitation/emission mechanism, and the astrophysical implications

2. A New Component of the Interstellar Matter: Small Grains and Large Aromatic Molecules

3. Polycyclic aromatic hydrocarbons and the unidentified infrared emission bands - Auto exhaust along the Milky Way

4. Vibrational spectroscopy of interstellar molecules

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