Looking at the photon-dominated region in NGC 2024 through FIR line emission

Astronomy and Astrophysics

Volumn 358, Issue 1, 2000, Pages 310-320

  Giannini, T ^a,b,c   Nisini, B ^a   Lorenzetti, D ^a,c   Di Giorgio, A M ^c   Spinoglio, L ^c   Benedettini, M ^c   Saraceno, P ^c   Smith, H A ^d   White, G J ^e,f  

^a INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^b SAPIENZA UNIVERSITY OF ROME   (Italy)

^c UNIVERSITY OF ROME TOR VERGATA   (Italy)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^e QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

^f STOCKHOLM OBSERVATORY   (Sweden)

Author keywords

Infrared: ISM: lines and bands; ISM: H II regions; ISM: individual objects: NGC 2024; Stars: formation

Indexed keywords

EID: 25544471972     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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