The temperature and ionization structure of the emitting gas in H II galaxies: implicatins for the accuracy of abundance determinations
Publisher
Oxford University PressDate
2006Citation
10.1111/j.1365-2966.2006.10856.x
Monthly Notices of the Royal Astronomical Society 372 (2006): 293-312
ISSN
1365-2966DOI
10.1111/j.1365-2966.2006.10856.xEditor's Version
http://dx.doi.org/10.1111/j.1365-2966.2006.10856.xSubjects
ISM: abundances; Galaxies: abundances; Galaxies: fundamental parameters; Galaxies: starburst; FísicaNote
This is an electronic version of an article published in Monthly Notices of the Royal Astronomical Society. Hägele, G.F., Pérez-Montero, E., Díaz, A.I., Terlevich, E. and R. Terlevich. The temperature and ionization structure of the emitting gas in H II galaxies: implicatins for the accuracy of abundance determinations. Monthly Notices of the Royal Astronomical Society 372 (2006): 293-312Rights
© Royal Astronomical SocietyFiles in this item
Google Scholar:Hägele, Guillermo F.
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Pérez Montero, Enrique
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Díaz Beltrán, Ángeles Isabel
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Terlevich, Elena
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Terlevich, Roberto