Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to now
We present a long-term project to study the characteristics and evolution of current star-forming galaxies at different redshifts. Our results support the idea that the higher Star Formation Density measured at redshift z=0.24 is due to an increase of the density of bursting galaxies and not to an i...
| Autores: | , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Fecha de publicación: | 2005 |
| País: | España |
| Institución: | Universidad Complutense de Madrid (UCM) |
| Repositorio: | Docta Complutense |
| Idioma: | inglés |
| OAI Identifier: | oai:docta.ucm.es:20.500.14352/52577 |
| Acceso en línea: | https://hdl.handle.net/20.500.14352/52577 |
| Access Level: | acceso abierto |
| Palabra clave: | 52 Astronomy Astrophysics Astrofísica Astronomía (Física) |
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Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to nowPascual Ramírez, SergioVillar, V.Gallego Maestro, JesúsZamorano Calvo, JaimePelló, R.Díaz-Guerra Viejo, CarlosAragón Salamanca, A.52AstronomyAstrophysicsAstrofísicaAstronomía (Física)We present a long-term project to study the characteristics and evolution of current star-forming galaxies at different redshifts. Our results support the idea that the higher Star Formation Density measured at redshift z=0.24 is due to an increase of the density of bursting galaxies and not to an intrinsic change on overall galaxy properties.Instituto de Astronomía de la UNAMUniversidad Complutense de Madrid20052005-01-0120052005-01-01journal articlehttp://purl.org/coar/resource_type/c_6501info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/20.500.14352/52577reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/525772026-06-02T12:44:21Z |
| dc.title.none.fl_str_mv |
Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to now |
| title |
Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to now |
| spellingShingle |
Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to now Pascual Ramírez, Sergio 52 Astronomy Astrophysics Astrofísica Astronomía (Física) |
| title_short |
Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to now |
| title_full |
Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to now |
| title_fullStr |
Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to now |
| title_full_unstemmed |
Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to now |
| title_sort |
Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to now |
| dc.creator.none.fl_str_mv |
Pascual Ramírez, Sergio Villar, V. Gallego Maestro, Jesús Zamorano Calvo, Jaime Pelló, R. Díaz-Guerra Viejo, Carlos Aragón Salamanca, A. |
| author |
Pascual Ramírez, Sergio |
| author_facet |
Pascual Ramírez, Sergio Villar, V. Gallego Maestro, Jesús Zamorano Calvo, Jaime Pelló, R. Díaz-Guerra Viejo, Carlos Aragón Salamanca, A. |
| author_role |
author |
| author2 |
Villar, V. Gallego Maestro, Jesús Zamorano Calvo, Jaime Pelló, R. Díaz-Guerra Viejo, Carlos Aragón Salamanca, A. |
| author2_role |
author author author author author author |
| dc.contributor.none.fl_str_mv |
Universidad Complutense de Madrid |
| dc.subject.none.fl_str_mv |
52 Astronomy Astrophysics Astrofísica Astronomía (Física) |
| topic |
52 Astronomy Astrophysics Astrofísica Astronomía (Física) |
| description |
We present a long-term project to study the characteristics and evolution of current star-forming galaxies at different redshifts. Our results support the idea that the higher Star Formation Density measured at redshift z=0.24 is due to an increase of the density of bursting galaxies and not to an intrinsic change on overall galaxy properties. |
| publishDate |
2005 |
| dc.date.none.fl_str_mv |
2005 2005-01-01 2005 2005-01-01 |
| dc.type.none.fl_str_mv |
journal article http://purl.org/coar/resource_type/c_6501 |
| dc.type.openaire.fl_str_mv |
info:eu-repo/semantics/article |
| format |
article |
| dc.identifier.none.fl_str_mv |
https://hdl.handle.net/20.500.14352/52577 |
| url |
https://hdl.handle.net/20.500.14352/52577 |
| dc.language.none.fl_str_mv |
Inglés eng |
| language_invalid_str_mv |
Inglés |
| language |
eng |
| dc.rights.none.fl_str_mv |
open access http://purl.org/coar/access_right/c_abf2 |
| dc.rights.openaire.fl_str_mv |
info:eu-repo/semantics/openAccess |
| rights_invalid_str_mv |
open access http://purl.org/coar/access_right/c_abf2 |
| eu_rights_str_mv |
openAccess |
| dc.format.none.fl_str_mv |
application/pdf |
| dc.publisher.none.fl_str_mv |
Instituto de Astronomía de la UNAM |
| publisher.none.fl_str_mv |
Instituto de Astronomía de la UNAM |
| dc.source.none.fl_str_mv |
reponame:Docta Complutense instname:Universidad Complutense de Madrid (UCM) |
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Universidad Complutense de Madrid (UCM) |
| reponame_str |
Docta Complutense |
| collection |
Docta Complutense |
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|
| repository.mail.fl_str_mv |
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1869425075110805504 |
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15,300724 |