The evolution of the observed Hubble sequence over the past 6GYR

During the past years we have confronted serious problems of methodology concerning the morphological and kinematic classification of distant galaxies. This has forced us to create a new simple and effective morphological classification methodology, in order to guarantee a morpho-kinematic correlati...

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Autor principal: Delgado, Rodney (author)
Altres autors: Hammer, Francois (author), Yang, Yan Bin (author), Puech, Mathieu (author), Flores, Héctor (author), Rodrígues, Myriam (author)
Format: article
Idioma:anglès
Publicat: 2010
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Accés en línia:http://ridda2.utp.ac.pa/handle/123456789/2882
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author Delgado, Rodney
author2 Hammer, Francois
Yang, Yan Bin
Puech, Mathieu
Flores, Héctor
Rodrígues, Myriam
author2_role author
author
author
author
author
author_browse Delgado, Rodney
Flores, Héctor
Hammer, Francois
Puech, Mathieu
Rodrígues, Myriam
Yang, Yan Bin
author_facet Delgado, Rodney
Hammer, Francois
Yang, Yan Bin
Puech, Mathieu
Flores, Héctor
Rodrígues, Myriam
author_role author
collection Repositorio Institucional de documento digitales de acceso abierto de la UTP
dc.creator.none.fl_str_mv Delgado, Rodney
Hammer, Francois
Yang, Yan Bin
Puech, Mathieu
Flores, Héctor
Rodrígues, Myriam
dc.date.none.fl_str_mv 2010-11-01
2010-11-01
2017-08-24T20:19:48Z
2017-08-24T20:19:48Z
2017-08-24T20:19:48Z
2017-08-24T20:19:48Z
dc.format.none.fl_str_mv application/pdf
dc.identifier.none.fl_str_mv http://ridda2.utp.ac.pa/handle/123456789/2882
http://ridda2.utp.ac.pa/handle/123456789/2882
dc.language.none.fl_str_mv eng
eng
dc.rights.none.fl_str_mv https://creativecommons.org/licenses/by-nc-sa/4.0/
info:eu-repo/semantics/openAccess
dc.source.none.fl_str_mv reponame:Repositorio Institucional de documento digitales de acceso abierto de la UTP
instname:Universidad Tecnológica de Panamá
instacron:U Tecnológica de Panamá
dc.subject.none.fl_str_mv galaxies
evolution-galaxies
formation-galaxies
peculiar-galaxies
spiralgalaxies
statistics methods
data analysis
galaxies
evolution-galaxies
formation-galaxies
peculiar-galaxies
spiralgalaxies
statistics methods
data analysis
dc.title.none.fl_str_mv The evolution of the observed Hubble sequence over the past 6GYR
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
description During the past years we have confronted serious problems of methodology concerning the morphological and kinematic classification of distant galaxies. This has forced us to create a new simple and effective morphological classification methodology, in order to guarantee a morpho-kinematic correlation, make the reproducibility easier and restrict the classification subjectivity. Giving the characteristic of our morphological classification, we have thus been able to apply the same methodology, using equivalent observations, to representative samples of local and distant galaxies. It has allowed us to derive, for the first time, the distant Hubble sequence (_6 Gyr ago), and determine a morphological evolution of galaxies over the past 6 Gyr. Our results strongly suggest that more than half of the present-day spirals had peculiar morphologies, 6 Gyr ago.
eu_rights_str_mv openAccess
format article
id PA_430abb2c00cc7cec1920078cbd0e0c97
instacron_str U Tecnológica de Panamá
institution U Tecnológica de Panamá
instname_str Universidad Tecnológica de Panamá
language eng
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network_name_str oai la ref anni2
oai_identifier_str oai:ridda2.utp.ac.pa:123456789/2882
publishDate 2010
publishDateSort 2010
reponame_str Repositorio Institucional de documento digitales de acceso abierto de la UTP
repository.mail.fl_str_mv
repository.name.fl_str_mv
repository_id_str
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/4.0/
spelling The evolution of the observed Hubble sequence over the past 6GYRDelgado, RodneyHammer, FrancoisYang, Yan BinPuech, MathieuFlores, HéctorRodrígues, Myriamgalaxiesevolution-galaxiesformation-galaxiespeculiar-galaxiesspiralgalaxiesstatistics methodsdata analysisgalaxiesevolution-galaxiesformation-galaxiespeculiar-galaxiesspiralgalaxiesstatistics methodsdata analysisDuring the past years we have confronted serious problems of methodology concerning the morphological and kinematic classification of distant galaxies. This has forced us to create a new simple and effective morphological classification methodology, in order to guarantee a morpho-kinematic correlation, make the reproducibility easier and restrict the classification subjectivity. Giving the characteristic of our morphological classification, we have thus been able to apply the same methodology, using equivalent observations, to representative samples of local and distant galaxies. It has allowed us to derive, for the first time, the distant Hubble sequence (_6 Gyr ago), and determine a morphological evolution of galaxies over the past 6 Gyr. Our results strongly suggest that more than half of the present-day spirals had peculiar morphologies, 6 Gyr ago.During the past years we have confronted serious problems of methodology concerning the morphological and kinematic classification of distant galaxies. This has forced us to create a new simple and effective morphological classification methodology, in order to guarantee a morpho-kinematic correlation, make the reproducibility easier and restrict the classification subjectivity. Giving the characteristic of our morphological classification, we have thus been able to apply the same methodology, using equivalent observations, to representative samples of local and distant galaxies. It has allowed us to derive, for the first time, the distant Hubble sequence (_6 Gyr ago), and determine a morphological evolution of galaxies over the past 6 Gyr. Our results strongly suggest that more than half of the present-day spirals had peculiar morphologies, 6 Gyr ago.2017-08-24T20:19:48Z2017-08-24T20:19:48Z2017-08-24T20:19:48Z2017-08-24T20:19:48Z2010-11-012010-11-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://ridda2.utp.ac.pa/handle/123456789/2882http://ridda2.utp.ac.pa/handle/123456789/2882engenghttps://creativecommons.org/licenses/by-nc-sa/4.0/info:eu-repo/semantics/openAccessreponame:Repositorio Institucional de documento digitales de acceso abierto de la UTPinstname:Universidad Tecnológica de Panamáinstacron:U Tecnológica de Panamáoai:ridda2.utp.ac.pa:123456789/28822021-07-06T15:35:11Z
spellingShingle The evolution of the observed Hubble sequence over the past 6GYR
Delgado, Rodney
galaxies
evolution-galaxies
formation-galaxies
peculiar-galaxies
spiralgalaxies
statistics methods
data analysis
galaxies
evolution-galaxies
formation-galaxies
peculiar-galaxies
spiralgalaxies
statistics methods
data analysis
status_str publishedVersion
title The evolution of the observed Hubble sequence over the past 6GYR
title_full The evolution of the observed Hubble sequence over the past 6GYR
title_fullStr The evolution of the observed Hubble sequence over the past 6GYR
title_full_unstemmed The evolution of the observed Hubble sequence over the past 6GYR
title_short The evolution of the observed Hubble sequence over the past 6GYR
title_sort The evolution of the observed Hubble sequence over the past 6GYR
topic galaxies
evolution-galaxies
formation-galaxies
peculiar-galaxies
spiralgalaxies
statistics methods
data analysis
galaxies
evolution-galaxies
formation-galaxies
peculiar-galaxies
spiralgalaxies
statistics methods
data analysis
url http://ridda2.utp.ac.pa/handle/123456789/2882