Infrared helium-hydrogen line ratios as a measure of stellar effective temperature

Monthly Notices of the Royal Astronomical Society

Volumn 320, Issue 1, 2001, Pages 83-102

  Lumsden, S L ^a,b   Puxley, P J ^c   Hoare, M G ^a  

^a UNIVERSITY OF LEEDS   (United Kingdom)

^b GEMINI OBSERVATORY   (United States)

^c ANGLO AUSTRALIAN OBSERVATORY   (Australia)

Author keywords

Infrared: ISM; Planetary nebulae: general

Indexed keywords

GALAXIES; INFRARED DEVICES; PHOTOIONIZATION; TEMPERATURE;

EFFECTIVE TEMPERATURE; HYDROGEN LINES; INFRARED: ISM; LINE RATIOS; NEAR INFRARED; NEAR-INFRARED; PHOTOIONIZATION MODELS; PLANETARY NEBULA; PLANETARY NEBULAE:GENERAL; STELLARS;

STARS;

EID: 0038233020     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.03954.x     Document Type: Article

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