[Fe II] 1.257 μm and He I 1.083 μm emission in the central region of the Orion Nebula: H II region, HH flows, jets, and proplyds

Astrophysical Journal

Volumn 566, Issue 2 I, 2002, Pages 910-924

  Takami, Michihiro ^a,b   Usuda, Tomonori ^c   Sugai, Hajime ^d   Suto, Hiroshi ^c   Pyo, Tae Soo ^a,c   Takeyama, Norihide ^a   Aoki, Tetsuo ^e   Mizutani, Kohei ^e   Tanaka, Masuo ^a  

^a UNIVERSITY OF TOKYO   (Japan)

^b UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^d KYOTO UNIVERSITY   (Japan)

^e NATIONAL INSTITUTE OF INFORMATION AND COMMUNICATIONS TECHNOLOGY   (Japan)

Author keywords

H II regions; Infrared: ISM; ISM: individual (Orion Nebula); Stars: formation

Indexed keywords

EID: 0042770378     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/338245     Document Type: Article

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