Emission and cooling by CO in interstellar shock waves

Monthly Notices of the Royal Astronomical Society

Volumn 395, Issue 1, 2009, Pages 234-239

  Flower, D R ^a   Gusdorf, A ^a,b,c  

^a DURHAM UNIVERSITY   (United Kingdom)

^b UNIVERSITÉ PARIS SUD   (France)

^c MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

Author keywords

Infrared: ISM; ISM: jets and outflows; ISM: molecules; Radiative transfer; Radio lines: ISM; Shock waves

Indexed keywords

COOLING; MOLECULES; POPULATION STATISTICS;

CO MOLECULE; INFRARED: ISM; ISM JETS AND OUTFLOWS; ISM:MOLECULES; RADIO LINES: ISM; ROTATIONAL LEVELS; SHOCK-WAVES; STATISTICAL EQUILIBRIUM; STEADY STATE; VELOCITY GRADIENTS;

SHOCK WAVES;

EID: 64549108948     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14569.x     Document Type: Article

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