Gas-phase C60Hn+q (n = 0–4, q = 0,1) fullerenes and fulleranes: spectroscopic simulations shed light on cosmic molecular structures-Reference-Cited by-同舟云学术

Gas-phase C₆₀H_n^+q (n = 0–4, q = 0,1) fullerenes and fulleranes: spectroscopic simulations shed light on cosmic molecular structures

Author:

Oliveira Ricardo R.¹^ORCID,Molpeceres Germán²^ORCID,Montserrat Ricardo¹^ORCID,Fantuzzi Felipe³^ORCID,Rocha Alexandre B.¹,Kästner Johannes⁴^ORCID

Affiliation:

1. Chemistry Institute, Federal University of Rio de Janeiro, Rio de Janeiro, Brazil

2. Department of Astronomy, Graduate School of Science, The University of Tokyo, Tokyo 113 0033, Japan

3. School of Chemistry and Forensic Science, University of Kent, Canterbury CT2 7NH, UK

4. Institute for Theoretical Chemistry, University of Stuttgart, Stuttgart, Germany

Abstract

Several hydrogenated fullerenes can absorb radiation in the near-IR region.

Funder

Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior

Japan Society for the Promotion of Science

Deutsche Forschungsgemeinschaft

Publisher

Royal Society of Chemistry (RSC)

Subject

Physical and Theoretical Chemistry,General Physics and Astronomy

Link

Reference74 articles.

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