Star formation driven galactic winds in UGC 10043

Lopez-Coba, C.; Sánchez, S.F.; Moiseev, A.V.; Oparin, D. V.; Bitsakis, T.; Cruz-González, Irene; Morisset, C.; Galbany, Lluís; Bland-Hawthorn, J.; Roth, M.M.; Dettmar, Ralf-Jürgen; Bomans, D. J.; González Delgado, Rosa M.; Cano-Díaz, M.; Marino, R.A.; Kehrig, C.; Monreal-Ibero, Ana; Abril-Melgarejo, V.

Star formation driven galactic winds in UGC 10043

We study the galactic wind in the edge-on spiral galaxy UGC 10043 with the combination of the CALIFA integral field spectroscopy data, scanning Fabry-Perot interferometry (FPI) and multiband photometry. We detect ionized gas in the extraplanar regions reaching a relatively high distance, up to ~4 kp...

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Authors:	Lopez-Coba, C., Sánchez, S.F., Moiseev, A.V., Oparin, D. V., Bitsakis, T., Cruz-González, Irene, Morisset, C., Galbany, Lluís, Bland-Hawthorn, J., Roth, M.M., Dettmar, Ralf-Jürgen, Bomans, D. J., González Delgado, Rosa M., Cano-Díaz, M., Marino, R.A., Kehrig, C., Monreal-Ibero, Ana, Abril-Melgarejo, V.
Format:	article
Status:	Published version
Publication Date:	2017
Country:	España
Institution:	Consejo Superior de Investigaciones Científicas (CSIC)
Repository:	DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:	oai:digital.csic.es:10261/376279
Online Access:	http://hdl.handle.net/10261/376279
Access Level:	Open access
Keyword:	ISM: jets and outflows Galaxies: individual: UGC 10043 Galaxies: ISM Galaxies: kinematics and dynamics.

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spelling	Star formation driven galactic winds in UGC 10043Lopez-Coba, C.Sánchez, S.F.Moiseev, A.V.Oparin, D. V.Bitsakis, T.Cruz-González, IreneMorisset, C.Galbany, LluísBland-Hawthorn, J.Roth, M.M.Dettmar, Ralf-JürgenBomans, D. J.González Delgado, Rosa M.Cano-Díaz, M.Marino, R.A.Kehrig, C.Monreal-Ibero, AnaAbril-Melgarejo, V.ISM: jets and outflowsGalaxies: individual: UGC 10043Galaxies: ISMGalaxies: kinematics and dynamics.We study the galactic wind in the edge-on spiral galaxy UGC 10043 with the combination of the CALIFA integral field spectroscopy data, scanning Fabry-Perot interferometry (FPI) and multiband photometry. We detect ionized gas in the extraplanar regions reaching a relatively high distance, up to ~4 kpc above the galactic disc. The ionized gas line ratios ([N II]/Hα, [S II]/Hα and [O I]/Hα) present an enhancement along the semiminor axis, in contrast with the values found at the disc, where they are compatible with ionization due to H ii-regions. These differences, together with the biconic symmetry of the extra-planar ionized structure, make UGC 10043 a clear candidate for a galaxy with gas outflows ionizated by shocks. From the comparison of shock models with the observed line ratios, and the kinematics observed from the FPI data, we constrain the physical properties of the observed outflow. The data are compatible with a velocity increase of the gas along the extraplanar distances up to <400 km s and the pre-shock density decreasing in the same direction. We also observe a discrepancy in the SFR estimated based on Hα (0.36 M yr) and that estimated with the cigale code, the latter being five times larger. Nevertheless, this SFR is still not enough to drive the observed galactic wind if we do not take into account the filling factor. We stress that the combination of the three techniques of observation with the models is a powerful tool to explore galactic winds in the Local Universe. © 2016 The AuthorsThe authors wish to thank an anonymous referee for his/her thorough review, and the valuable suggestions and comments which significantly contributed to improve the quality of the publication. CALIFA is the first legacy survey being performed at Calar Alto. The CALIFA collaboration would like to thank IAA-CSIC and MPIA-MPG as major partners of the observatory, and CAHA itself, for the unique access to telescope time and support in manpower and infrastructures. The CALIFA collaboration thanks also the CAHA staff for the dedication to this project. We thank CONACYT-125180, DGAPA(UNAM)-IA100815 and DGAPA(UNAM)-IN107215 projects and the institutions (CONACYT and DGAPA-UNAM) for providing financial support for this study. The Fabry–Perot observations were obtained with the 6-m tele- ´ scope of the Special Astrophysical Observatory of the Russian Academy of Sciences, and were carried out with the financial support of the Ministry of Education and Science of the Russian Federation (Contract No. N14.619.21.0004 for the project RFMEFI61914X0004). AVM and DVO are also grateful for the financial support via grant MD3623.2015.2 from the President of the Russian Federation. L.G. was supported in part by the US National Science Foundation under Grant AST-1311862. RAM acknowledges support by the Swiss National Science Foundation.Oxford University PressConsejo Nacional de Ciencia y Tecnología (México)Universidad Nacional Autónoma de MéxicoMinistry of Education and Science of the Russian FederationNational Science Foundation (US)Swiss National Science FoundationConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2025202520172025info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/376279reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Ingléshttp://dx.doi.org/10.1093/mnras/stw3355Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3762792026-05-22T06:33:51Z
dc.title.none.fl_str_mv	Star formation driven galactic winds in UGC 10043
title	Star formation driven galactic winds in UGC 10043
spellingShingle	Star formation driven galactic winds in UGC 10043 Lopez-Coba, C. ISM: jets and outflows Galaxies: individual: UGC 10043 Galaxies: ISM Galaxies: kinematics and dynamics.
title_short	Star formation driven galactic winds in UGC 10043
title_full	Star formation driven galactic winds in UGC 10043
title_fullStr	Star formation driven galactic winds in UGC 10043
title_full_unstemmed	Star formation driven galactic winds in UGC 10043
title_sort	Star formation driven galactic winds in UGC 10043
dc.creator.none.fl_str_mv	Lopez-Coba, C. Sánchez, S.F. Moiseev, A.V. Oparin, D. V. Bitsakis, T. Cruz-González, Irene Morisset, C. Galbany, Lluís Bland-Hawthorn, J. Roth, M.M. Dettmar, Ralf-Jürgen Bomans, D. J. González Delgado, Rosa M. Cano-Díaz, M. Marino, R.A. Kehrig, C. Monreal-Ibero, Ana Abril-Melgarejo, V.
author	Lopez-Coba, C.
author_facet	Lopez-Coba, C. Sánchez, S.F. Moiseev, A.V. Oparin, D. V. Bitsakis, T. Cruz-González, Irene Morisset, C. Galbany, Lluís Bland-Hawthorn, J. Roth, M.M. Dettmar, Ralf-Jürgen Bomans, D. J. González Delgado, Rosa M. Cano-Díaz, M. Marino, R.A. Kehrig, C. Monreal-Ibero, Ana Abril-Melgarejo, V.
author_role	author
author2	Sánchez, S.F. Moiseev, A.V. Oparin, D. V. Bitsakis, T. Cruz-González, Irene Morisset, C. Galbany, Lluís Bland-Hawthorn, J. Roth, M.M. Dettmar, Ralf-Jürgen Bomans, D. J. González Delgado, Rosa M. Cano-Díaz, M. Marino, R.A. Kehrig, C. Monreal-Ibero, Ana Abril-Melgarejo, V.
author2_role	author author author author author author author author author author author author author author author author author
dc.contributor.none.fl_str_mv	Consejo Nacional de Ciencia y Tecnología (México) Universidad Nacional Autónoma de México Ministry of Education and Science of the Russian Federation National Science Foundation (US) Swiss National Science Foundation Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv	ISM: jets and outflows Galaxies: individual: UGC 10043 Galaxies: ISM Galaxies: kinematics and dynamics.
topic	ISM: jets and outflows Galaxies: individual: UGC 10043 Galaxies: ISM Galaxies: kinematics and dynamics.
description	We study the galactic wind in the edge-on spiral galaxy UGC 10043 with the combination of the CALIFA integral field spectroscopy data, scanning Fabry-Perot interferometry (FPI) and multiband photometry. We detect ionized gas in the extraplanar regions reaching a relatively high distance, up to ~4 kpc above the galactic disc. The ionized gas line ratios ([N II]/Hα, [S II]/Hα and [O I]/Hα) present an enhancement along the semiminor axis, in contrast with the values found at the disc, where they are compatible with ionization due to H ii-regions. These differences, together with the biconic symmetry of the extra-planar ionized structure, make UGC 10043 a clear candidate for a galaxy with gas outflows ionizated by shocks. From the comparison of shock models with the observed line ratios, and the kinematics observed from the FPI data, we constrain the physical properties of the observed outflow. The data are compatible with a velocity increase of the gas along the extraplanar distances up to <400 km s and the pre-shock density decreasing in the same direction. We also observe a discrepancy in the SFR estimated based on Hα (0.36 M yr) and that estimated with the cigale code, the latter being five times larger. Nevertheless, this SFR is still not enough to drive the observed galactic wind if we do not take into account the filling factor. We stress that the combination of the three techniques of observation with the models is a powerful tool to explore galactic winds in the Local Universe. © 2016 The Authors
publishDate	2017
dc.date.none.fl_str_mv	2017 2025 2025 2025
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/10261/376279
url	http://hdl.handle.net/10261/376279
dc.language.none.fl_str_mv	Inglés
language_invalid_str_mv	Inglés
dc.relation.none.fl_str_mv	http://dx.doi.org/10.1093/mnras/stw3355 Sí
dc.rights.none.fl_str_mv	info:eu-repo/semantics/openAccess
eu_rights_str_mv	openAccess
dc.publisher.none.fl_str_mv	Oxford University Press
publisher.none.fl_str_mv	Oxford University Press
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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score	15,81155

Star formation driven galactic winds in UGC 10043

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