Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-29T11:31:47.369Z Has data issue: false hasContentIssue false

Physical conditions in H II galaxies

Published online by Cambridge University Press:  26 May 2016

Carolina Kehrig
Affiliation:
Observatório Nacional, Rua General José Cristino 77, Sao Cristovao, 20921-400 Rio de Janeiro, Brasil
Eduardo Telles
Affiliation:
Observatório Nacional, Rua General José Cristino 77, Sao Cristovao, 20921-400 Rio de Janeiro, Brasil
François Cuisinier
Affiliation:
Departamento de Astronomia, Universidade Federal do Rio de Janeiro, 20080-090 Rio de Janeiro, Brasil

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present a spectrophotometric survey of 111 H ii galaxies. Observations were made at the ESO 1.52m telescope, with the b&c spectrograph. Our sample presents a great overlap with Terlevich et al. 1991. Additional targets come from the Calan-Tololo an Marseille catalogues. All objects have been observed and analysed homogeneously. We analyse their statistical properties and derive physical conditions (reddening, electron temperature, electron density), as well as chemical abundances.

Type
Part 4. Feedback from Massive Stars
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Maza, J., Ruiz, M.T., Gonzalez, L.E., Wischnjewsky, M., Peña, M. 1991, A&AS 89, 389 (Calán-Tololo Survey III — H ii Galaxies).Google Scholar
Surace, C., Conte, G. 1998, A&AS 133, 171 (Marseille Schmidt Survey).Google Scholar
Terlevich, R., Melnick, J., Masegosa, J., Moles, M., Copetti, M.V.F. 1991, A&AS 91, 285.Google Scholar