Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxies

We derive rotation curves, surface brightness profiles, and oxygen abundance distributions for 147 late-type galaxies using the publicly available spectroscopy obtained by the MaNGA survey. Changes of the central oxygen abundance (O/H)0, the abundance at the optical radius (O/H)R25, and the abundanc...

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Detalles Bibliográficos
Autores: Pilyugin, L.S., Grebel, E.K., Zinchenko, I.A., Nefedyev, Y.A., Vílchez Medina, José Manuel
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2019
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/189621
Acceso en línea:http://hdl.handle.net/10261/189621
Access Level:acceso abierto
Palabra clave:Galaxies: abundances
Galaxies: ISM
Galaxies: kinematics and dynamics
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spelling Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxiesPilyugin, L.S.Grebel, E.K.Zinchenko, I.A.Nefedyev, Y.A.Vílchez Medina, José ManuelGalaxies: abundancesGalaxies: ISMGalaxies: kinematics and dynamicsWe derive rotation curves, surface brightness profiles, and oxygen abundance distributions for 147 late-type galaxies using the publicly available spectroscopy obtained by the MaNGA survey. Changes of the central oxygen abundance (O/H)0, the abundance at the optical radius (O/H)R25, and the abundance gradient with rotation velocity Vrot were examined for galaxies with rotation velocities from 90 km s to 350 km s. We find that each relation shows a break at Vrot ∼ 200 km s. The central (O/H)0 abundance increases with rising Vrot and the slope of the (O/H)0-Vrot relation is steeper for galaxies with Vrot Vrot. The mean scatter of the central abundances around this relation is 0.053 dex. The relation between the abundance at the optical radius of a galaxy and its rotation velocity is similar; the mean scatter in abundances around this relation is 0.081 dex. The radial abundance gradient expressed in dex/kpc flattens with the increase of the rotation velocity. The slope of the relation is very low for galaxies with Vrot Vrot. The abundance gradient expressed in dex/R25 is roughly constant for galaxies with Vrot Vrot, flattens towards Vrot, and then again is roughly constant for galaxies with Vrot Vrot. The change of the gradient expressed in terms of dex/hd (where hd is the disc scale length), in terms of dex/Re, d (where Re, d is the disc effective radius), and in terms of dex/Re, g (where Re, g is the galaxy effective radius) with rotation velocity is similar to that for gradient in dex/R25. The relations between abundance characteristics and other basic parameters (stellar mass, luminosity, and radius) are also considered.I.A.Z. acknowledge support within the framework of Sonderforschungsbereich (SFB 881) on >The Milky Way System> (especially subproject A05), which is funded by the German Research Foundation (DFG). L.S.P. and I.A.Z. thank for their hospitality of the Astronomisches Rechen-Institut at Heidelberg University, where part of this investigation was carried out. I.A.Z. acknowledges the support of the Volkswagen Foundation under the Trilateral Partnerships grant No. 90411. I.A.Z. acknowledges the support by the Ukrainian National Grid project (especially subproject 400Kt) of the NAS of Ukraine. J.M.V acknowledges financial support from projects AYA2017-79724-C4-4-P, of the Spanish PNAYA, and Junta de Andalucia Excellence PEX2011-FQM705. This work was partly funded by the subsidy allocated to Kazan Federal University for the state assignment in the sphere of scientific activities (L.S.P.).EDP SciencesGerman Research FoundationVolkswagen FoundationNational Academy of Sciences of UkraineMinisterio de Economía y Competitividad (España)Junta de AndalucíaKazan Federal UniversityConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2019201920192019info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/189621reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2017-79724-C4-4-Phttp://doi.org/10.1051/0004-6361/201834239Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/1896212026-05-22T06:33:51Z
dc.title.none.fl_str_mv Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxies
title Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxies
spellingShingle Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxies
Pilyugin, L.S.
Galaxies: abundances
Galaxies: ISM
Galaxies: kinematics and dynamics
title_short Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxies
title_full Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxies
title_fullStr Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxies
title_full_unstemmed Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxies
title_sort Relations between abundance characteristics and rotation velocity for star-forming MaNGA galaxies
dc.creator.none.fl_str_mv Pilyugin, L.S.
Grebel, E.K.
Zinchenko, I.A.
Nefedyev, Y.A.
Vílchez Medina, José Manuel
author Pilyugin, L.S.
author_facet Pilyugin, L.S.
Grebel, E.K.
Zinchenko, I.A.
Nefedyev, Y.A.
Vílchez Medina, José Manuel
author_role author
author2 Grebel, E.K.
Zinchenko, I.A.
Nefedyev, Y.A.
Vílchez Medina, José Manuel
author2_role author
author
author
author
dc.contributor.none.fl_str_mv German Research Foundation
Volkswagen Foundation
National Academy of Sciences of Ukraine
Ministerio de Economía y Competitividad (España)
Junta de Andalucía
Kazan Federal University
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Galaxies: abundances
Galaxies: ISM
Galaxies: kinematics and dynamics
topic Galaxies: abundances
Galaxies: ISM
Galaxies: kinematics and dynamics
description We derive rotation curves, surface brightness profiles, and oxygen abundance distributions for 147 late-type galaxies using the publicly available spectroscopy obtained by the MaNGA survey. Changes of the central oxygen abundance (O/H)0, the abundance at the optical radius (O/H)R25, and the abundance gradient with rotation velocity Vrot were examined for galaxies with rotation velocities from 90 km s to 350 km s. We find that each relation shows a break at Vrot ∼ 200 km s. The central (O/H)0 abundance increases with rising Vrot and the slope of the (O/H)0-Vrot relation is steeper for galaxies with Vrot Vrot. The mean scatter of the central abundances around this relation is 0.053 dex. The relation between the abundance at the optical radius of a galaxy and its rotation velocity is similar; the mean scatter in abundances around this relation is 0.081 dex. The radial abundance gradient expressed in dex/kpc flattens with the increase of the rotation velocity. The slope of the relation is very low for galaxies with Vrot Vrot. The abundance gradient expressed in dex/R25 is roughly constant for galaxies with Vrot Vrot, flattens towards Vrot, and then again is roughly constant for galaxies with Vrot Vrot. The change of the gradient expressed in terms of dex/hd (where hd is the disc scale length), in terms of dex/Re, d (where Re, d is the disc effective radius), and in terms of dex/Re, g (where Re, g is the galaxy effective radius) with rotation velocity is similar to that for gradient in dex/R25. The relations between abundance characteristics and other basic parameters (stellar mass, luminosity, and radius) are also considered.
publishDate 2019
dc.date.none.fl_str_mv 2019
2019
2019
2019
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/189621
url http://hdl.handle.net/10261/189621
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv #PLACEHOLDER_PARENT_METADATA_VALUE#
info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2017-79724-C4-4-P
http://doi.org/10.1051/0004-6361/201834239
Sí
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
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