H2 emission from shocks in molecular outflows: The significance of departures from a stationary state

Monthly Notices of the Royal Astronomical Society

Volumn 308, Issue 1, 1999, Pages 271-280

  Flower, D R ^a   Pineau Des Forets G ^b  

^a DURHAM UNIVERSITY   (United Kingdom)

^b OBSERVATOIRE DE PARIS   (France)

Author keywords

ISM: individual: Cepheus A West; ISM: jets and outflows; ISM: molecules; Molecular processes; Shock waves; Stars: formation

Indexed keywords

EMISSION SPECTROSCOPY; MOLECULES; SILICON COMPOUNDS; STARS;

ISM JETS AND OUTFLOWS; ISM: INDIVIDUAL: CEPHEI A WEST; ISM: INDIVIDUALS; ISM:MOLECULES; MOLECULAR OUTFLOWS; MOLECULAR PROCESS; SHOCK-WAVES; STARS FORMATION; STATIONARY STATE; TIME DEPENDENCE;

SHOCK WAVES;

EID: 0000186911     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02729.x     Document Type: Article

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