Photoionization and evolutionary synthesis models for giant H ii regions |
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| Institution: | 1. Astronomy Centre, Sussex University, Falmer, Brighton, UK, BN1 9QH;2. Astrophysics, Blackett Labs, ICSTM, Prince Consort Rd, London SW7 2BZ UK;3. Institute of Astronomy, Madingley Rd, Cambridge, UK, CB3 OHA;1. CEH Monks Wood, Abbots Ripton, Huntingdon, Cambridgeshire PE28 2LS, UK;2. Department of Plant and Soil Science, Cruickshank Building, University of Aberdeen, Aberdeen AB24 3UU, UK;3. Department of Molecular and Cell Biology, Institute of Medical Sciences, Foresterhill, University of Aberdeen, Aberdeen AB25 2ZD, UK;1. Animal Science Research Institute, Southern Yangtse University(Wuxi University of Light Industry), Wuxi 214036, People''s Republic of China;2. Department of Molecular Biology, University of Gdańsk, Kladki 24, 80-822 Gdańsk, Poland;1. Indian Institute of Astrophysics, II Block, Koramangala P.O., Bangalore 560034, India;2. Physics Department, University College Cork, Cork, Ireland;3. Astro Space Center, Lebedev Physical Institute, Moscow, Russia |
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| Abstract: | We review the current stellar population synthesis models that are used for modeling giant H ii regions. Then we present some of the recent applications of photoionization models to the study of giant H ii regions, with particular emphasis on the electron temperature problem. |
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