Temperature variations from Hubble Space Telescope spectroscopy of the Orion Nebula

Monthly Notices of the Royal Astronomical Society

Volumn 340, Issue 2, 2003, Pages 362-374

  Rubin, R H ^a,b   Martin, P G ^c   Dufour, R J ^d   Ferland, G J ^e   Blagrave, K P M ^c   Liu, X W ^f   Nguyen, J F ^a   Baldwin, J A ^g  

^a NASA AMES RESEARCH CENTER   (United States)

^b Orion Enterprises   (United States)

^c UNIVERSITY OF TORONTO   (Canada)

^d RICE UNIVERSITY   (United States)

^e UNIVERSITY OF KENTUCKY   (United States)

^f PEKING UNIVERSITY   (China)

^g MICHIGAN STATE UNIVERSITY   (United States)

Author keywords

H ii regions; Ism: Abundances; Ism: Atoms; Ism: Individual: Ngc 1976; Ism: Individual: Proplyd p159 350

Indexed keywords

CARRIER CONCENTRATION; ELECTRON DENSITY MEASUREMENT; ELECTRONS; IONIZATION; SPACE TELESCOPES;

H II REGION; HUBBLE SPACE TELESCOPES; ISM: ABUNDANCE; ISM: ATOMS; ISM: INDIVIDUAL: NGC 1976; ISM: INDIVIDUAL: PROPLYD P159-350; ISM: INDIVIDUALS; LINE RATIOS; TEMPERATURE VARIATION;

TEMPERATURE DISTRIBUTION;

EID: 0041841807     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06185.x     Document Type: Article

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