The 'soot line': Destruction of presolar polycyclic aromatic hydrocarbons in the terrestrial planet-forming region of disks

Advances in Space Research

Volumn 46, Issue 1, 2010, Pages 44-49

  Kress, Monika E ^a   Tielens, Alexander G G M ^b   Frenklach, Michael ^c  

^a SAN JOSE STATE UNIVERSITY   (United States)

^b LEIDEN UNIVERSITY   (Netherlands)

^c UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Chemical model; PAH; Presolar organics; Protoplanetary disk; Solar nebula

Indexed keywords

CARBON; HYDROCARBONS; PLANETS; SOOT;

CHEMICAL MODEL; INTERSTELLAR MATERIALS; INTERSTELLAR MEDIUMS; ORGANICS; POLYCYCLIC AROMATIC HYDROCARBONS (PAHS); PROTOPLANETARY DISKS; SOLAR NEBULA; THERMAL DESTRUCTION;

POLYCYCLIC AROMATIC HYDROCARBONS;

EID: 79955052010     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2010.02.004     Document Type: Article

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