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Authors:
Sánchez, S. F
| Pérez, E
| Mendoza, M. A
| Papaderos, P
| Ellis, S
| Galbany, L
| Kehrig, C
| Monreal-Ibero, A
| González Delgado, R
| Mollá, M
| Ziegler, B
| de Lorenzo-Cáceres, A
| Rosales-Ortega, F. F
| Mendez-Abreu, J
| Bland-Hawthorn, J
| Bekeraitė, S
| Roth, M. M
| Pasquali, A
| Díaz, A
| Bomans, D
| van de Ven, G
| Wisotzki, L
| CALIFA collaboration,
| Miralles-Caballero, D
| López-Sánchez, A. R
| Iglesias-Páramo, J
| Marino, R. A
| Sánchez-Menguiano, L
| García-Benito, R
| Mast, D
Date: 2015
Subject Keyword:
galaxies: abundances
| galaxies: star formation
| galaxies: evolution
| galaxies: ISM
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/1260209
Description:
Context. H II regions in galaxies are the sites of star formation, so they are special places for understanding the build-up of stellar mass in the universe. The line ratios of this ionized gas are fr
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Authors:
Sanchez, S. F
| Kennicutt, R. C
| Alonso-Herrero, A
| Alves, J
| Bakos, J
| Bartáková, T
| Bland-Hawthorn, J
| Boselli, A
| Bomans, D. J
| Castillo-Morales, A
| Cortijo-Ferrero, C
| de Lorenzo-Cáceres, A
| Gil de Paz, A
| del Olmo, A
| Dettmar, R. - J
| Díaz, A
| Ellis, S
| Falcón-Barroso, J
| Flores, H
| Gallazzi, A
| García-Lorenzo, B
| González Delgado, R
| Gruel, N
| van de Ven, G
| Haines, T
| Hao, C
| Husemann, B
| Iglésias-Páramo, J
| Jahnke, K
| Johnson, B
| Jungwiert, B
| Kalinova, V
| Kehrig, C
| Kupko, D
| Vilchez, J. M
| López-Sánchez, Á. R
| Lyubenova, M
| Marino, R. A
| Mármol-Queraltó, E
| Márquez, I
| Masegosa, J
| Meidt, S
| Mendez-Abreu, J
| Monreal-Ibero, A
| Montijo, C
| Wisotzki, L
| Mourao, A. M
| Palacios-Navarro, G
| Papaderos, P
| Pasquali, A
| Peletier, R
| Pérez, E
| Pérez, I
| Quirrenbach, A
| Relaño, M
| Rosales-Ortega, F. F
| Walcher, C. J
| Roth, M. M
| Ruiz-Lara, T
| Sanchez-Blazquez, P
| Sengupta, C
| Singh, R
| Stanishev, V
| Trager, S. C
| Vazdekis, A
| Viironen, K
| Wild, V
| Mast, D
| Zibetti, S
| Ziegler, B
| Aguerri, J. A. L
| Albiol-Pérez, S
Date: 2012
Subject Keyword:
020100 Astronomical and Space Sciences
| galaxies: active
| galaxies: evolution
| galaxies: ISM
| galaxies: stellar content
| surveys; techniques
| spectroscopic
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/178171
Description:
The final product of galaxy evolution through cosmic time is the population of galaxies in the local universe. These galaxies are also those that can be studied in most detail, thus providing a string
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Authors:
Sánchez, S. F
| Rosales-Ortega, F. F
| Bland-Hawthorn, J
| Pérez, E
| González Delgado, R
| Husemann, B
| López-Sánchez, A. R
| Cid Fernandes, R
| Kehrig, C
| Walcher, C. J
| Gil De Paz, A
| Ellis, S
| Marino, R. A
| Iglesias-Páramo, J
| Vilchez, J. M
| Kennicutt, R. C
| Díaz, A. I
| Mast, D
| Monreal-Ibero, A
| García-Benito, R
Date: 2012
Subject Keyword:
020100 Astronomical and Space Sciences
| Galaxies: abundances
| Galaxies: evolution
| Galaxies: fundamental parameters
| Galaxies: ISM
| Galaxies: spiral
| Galaxies: star formation
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/200677
Description:
We analyse the spectroscopic properties of thousands of H ii regions identified in 38 face-on spiral galaxies. All galaxies were observed out to 2.4 effective radii using integral field spectroscopy (
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