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The chemical abundances in a sample of dwarf irregular galaxies II. The case of IC 4662 and ESO 245-G05
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2001 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 369, no 3, 797-811 p.Article in journal (Refereed) Published
Abstract [en]

Optical spectra of HII regions of two dwarf irregular galaxies are presented. The objects are IC 4662 and ESO 245-G05. Chemical abundances were derived in all the HII regions where the forbidden oxygen line [OIII]lambda 4363 Angstrom was detected. For spe

Place, publisher, year, edition, pages
E D P SCIENCES , 2001. Vol. 369, no 3, 797-811 p.
Keyword [en]
galaxies : evolution; galaxies : irregular; galaxies : stellar content; interstellar medium : HII regions : general; galaxies : individual : IC 4662; ESO 245-G05; BLUE COMPACT GALAXIES; STAR-FORMATION; OXYGEN ABUNDANCES; SPIRAL GALAXIES; EVOLUTION; EMISSI
URN: urn:nbn:se:uu:diva-36636OAI: oai:DiVA.org:uu-36636DiVA: diva2:64535
Addresses: Hidalgo-Gamez AM, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Astron Observ, S-75120 Uppsala, Sweden. CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-13

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