The Low-luminosity Galaxy Population in the NGC 5044 Group

Autores
Cellone, Sergio Aldo; Buzzoni, Alberto; Saviane, Ivo; Ivanov, Valentin D.; Borissova, Jordanka
Año de publicación
2007
Idioma
inglés
Tipo de recurso
parte de libro
Estado
versión publicada
Descripción
Detailed surface photometry for 79 (mostly dwarf) galaxies in the NGC 5044 Group area is analysed, revealing the existence of different morphologies among objects originally classified as early-type dwarfs. Particularly, a significant fraction of bright dwarf “ellipticals” show a distinct bulge+disc structure; we thus re-classify these objects as dwarf lenticulars (dS0). Our finding points at a possible scenario where these systems are the remnants of “harassed” disc galaxies. This is emphasized by the discovery of a few objects with hints for very low-surface brightness spiral-like structure. The colours, structure, and spatial distribution of the different galaxy types suggest that our classification may indeed be separating objects with different origins and/or evolutionary paths.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
Disc galaxy
Disc structure
Star formation history
Photometric redshift
Galaxy distribution
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/123909
Acceder
id SEDICI_8ea402c252a8a751c5b8b19079521a07
oai_identifier_str oai:sedici.unlp.edu.ar:10915/123909
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling The Low-luminosity Galaxy Population in the NGC 5044 GroupCellone, Sergio AldoBuzzoni, AlbertoSaviane, IvoIvanov, Valentin D.Borissova, JordankaCiencias AstronómicasDisc galaxyDisc structureStar formation historyPhotometric redshiftGalaxy distributionDetailed surface photometry for 79 (mostly dwarf) galaxies in the NGC 5044 Group area is analysed, revealing the existence of different morphologies among objects originally classified as early-type dwarfs. Particularly, a significant fraction of bright dwarf “ellipticals” show a distinct bulge+disc structure; we thus re-classify these objects as dwarf lenticulars (dS0). Our finding points at a possible scenario where these systems are the remnants of “harassed” disc galaxies. This is emphasized by the discovery of a few objects with hints for very low-surface brightness spiral-like structure. The colours, structure, and spatial distribution of the different galaxy types suggest that our classification may indeed be separating objects with different origins and/or evolutionary paths.Facultad de Ciencias Astronómicas y GeofísicasSpringer2007info:eu-repo/semantics/bookPartinfo:eu-repo/semantics/publishedVersionCapitulo de librohttp://purl.org/coar/resource_type/c_3248info:ar-repo/semantics/parteDeLibroapplication/pdf91-95http://sedici.unlp.edu.ar/handle/10915/123909enginfo:eu-repo/semantics/altIdentifier/isbn/978-3-540-71172-8info:eu-repo/semantics/altIdentifier/isbn/978-3-540-71173-5info:eu-repo/semantics/altIdentifier/doi/10.1007/978-3-540-71173-5_14info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:29:29Zoai:sedici.unlp.edu.ar:10915/123909Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:29:29.81SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv The Low-luminosity Galaxy Population in the NGC 5044 Group
title The Low-luminosity Galaxy Population in the NGC 5044 Group
spellingShingle The Low-luminosity Galaxy Population in the NGC 5044 Group
Cellone, Sergio Aldo
Ciencias Astronómicas
Disc galaxy
Disc structure
Star formation history
Photometric redshift
Galaxy distribution
title_short The Low-luminosity Galaxy Population in the NGC 5044 Group
title_full The Low-luminosity Galaxy Population in the NGC 5044 Group
title_fullStr The Low-luminosity Galaxy Population in the NGC 5044 Group
title_full_unstemmed The Low-luminosity Galaxy Population in the NGC 5044 Group
title_sort The Low-luminosity Galaxy Population in the NGC 5044 Group
dc.creator.none.fl_str_mv Cellone, Sergio Aldo
Buzzoni, Alberto
Saviane, Ivo
Ivanov, Valentin D.
Borissova, Jordanka
author Cellone, Sergio Aldo
author_facet Cellone, Sergio Aldo
Buzzoni, Alberto
Saviane, Ivo
Ivanov, Valentin D.
Borissova, Jordanka
author_role author
author2 Buzzoni, Alberto
Saviane, Ivo
Ivanov, Valentin D.
Borissova, Jordanka
author2_role author
author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Disc galaxy
Disc structure
Star formation history
Photometric redshift
Galaxy distribution
topic Ciencias Astronómicas
Disc galaxy
Disc structure
Star formation history
Photometric redshift
Galaxy distribution
dc.description.none.fl_txt_mv Detailed surface photometry for 79 (mostly dwarf) galaxies in the NGC 5044 Group area is analysed, revealing the existence of different morphologies among objects originally classified as early-type dwarfs. Particularly, a significant fraction of bright dwarf “ellipticals” show a distinct bulge+disc structure; we thus re-classify these objects as dwarf lenticulars (dS0). Our finding points at a possible scenario where these systems are the remnants of “harassed” disc galaxies. This is emphasized by the discovery of a few objects with hints for very low-surface brightness spiral-like structure. The colours, structure, and spatial distribution of the different galaxy types suggest that our classification may indeed be separating objects with different origins and/or evolutionary paths.
Facultad de Ciencias Astronómicas y Geofísicas
description Detailed surface photometry for 79 (mostly dwarf) galaxies in the NGC 5044 Group area is analysed, revealing the existence of different morphologies among objects originally classified as early-type dwarfs. Particularly, a significant fraction of bright dwarf “ellipticals” show a distinct bulge+disc structure; we thus re-classify these objects as dwarf lenticulars (dS0). Our finding points at a possible scenario where these systems are the remnants of “harassed” disc galaxies. This is emphasized by the discovery of a few objects with hints for very low-surface brightness spiral-like structure. The colours, structure, and spatial distribution of the different galaxy types suggest that our classification may indeed be separating objects with different origins and/or evolutionary paths.
publishDate 2007
dc.date.none.fl_str_mv 2007
dc.type.none.fl_str_mv info:eu-repo/semantics/bookPart
info:eu-repo/semantics/publishedVersion
Capitulo de libro
http://purl.org/coar/resource_type/c_3248
info:ar-repo/semantics/parteDeLibro
format bookPart
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/123909
url http://sedici.unlp.edu.ar/handle/10915/123909
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/isbn/978-3-540-71172-8
info:eu-repo/semantics/altIdentifier/isbn/978-3-540-71173-5
info:eu-repo/semantics/altIdentifier/doi/10.1007/978-3-540-71173-5_14
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
91-95
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
_version_ 1844616174182072320
score 13.070432

Publicaciones similares