The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence

Autores
Colombo, D.; Kalinova, V.; Utomo, D.; Rosolowsky, E.; Bolatto, A. D.; Levy, R. C.; Wong, T.; Sanchez, S. F.; Leroy, A. K.; Ostriker, E.; Blitz, L.; Vogel, S.; Mast, Damian; García Benito, Rubén; Husemann, Bernd; Dannerbauer, H.; Ellmeier, L.; Cao, Y.
Año de publicación
2018
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present a kpc-scale analysis of the relationship between the molecular depletion time (τdepmol ) and the orbital time (τorb) across the field of 39 face-on local galaxies, selected from the EDGE-CALIFA sample. We find that, on average, 5 per cent of the available molecular gas is converted into stars per orbital time, or τ depmol ~ 20 τorb. The resolved relation shows a scatter of ~0.5 dex. The scatter is ascribable to galaxies of different morphologies that follow different τ depmol -τorb relations which decrease in steepness from early- to late types. The morphologies appear to be linked with the star formation rate surface density, the molecular depletion time, and the orbital time, but they do not correlate with the molecular gas content of the galaxies in our sample.We speculate that in our molecular gas rich, early-type galaxies, the morphological quenching (in particular the disc stabilization via shear), rather than the absence of molecular gas, is the main factor responsible for their current inefficient star formation.
Fil: Colombo, D.. Max Planck Institut Fur Astronomie; Alemania
Fil: Kalinova, V.. Max Planck Institut Fur Astronomie; Alemania
Fil: Utomo, D.. University Of California At Los Angeles. Department Of Physics And Astronomy.; Estados Unidos. Ohio State University; Estados Unidos
Fil: Rosolowsky, E.. University of Alberta; Canadá
Fil: Bolatto, A. D.. University of Maryland; Estados Unidos
Fil: Levy, R. C.. University of Maryland; Estados Unidos
Fil: Wong, T.. Southern Illinois University. Department Of Physics; Estados Unidos
Fil: Sanchez, S. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; México
Fil: Leroy, A. K.. Ohio University; Estados Unidos
Fil: Ostriker, E.. University of Princeton; Estados Unidos
Fil: Blitz, L.. Berkeley University; Estados Unidos
Fil: Vogel, S.. University of Maryland; Estados Unidos
Fil: Mast, Damian. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: García Benito, Rubén. Instituto de Astrofísica de Andalucía; España
Fil: Husemann, Bernd. Max Planck Institut Fur Astronomie; Alemania
Fil: Dannerbauer, H.. Universidad de La Laguna; España
Fil: Ellmeier, L.. Vienna University of Technology; Austria
Fil: Cao, Y.. University of Illinois; Estados Unidos
Materia
GALAXIES: EVOLUTION
GALAXIES: KINEMATICS AND DYNAMICS
GALAXIES: STAR FORMATION
GALAXIES: STRUCTURE
ISM: MOLECULES
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/134608
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/134608
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequenceColombo, D.Kalinova, V.Utomo, D.Rosolowsky, E.Bolatto, A. D.Levy, R. C.Wong, T.Sanchez, S. F.Leroy, A. K.Ostriker, E.Blitz, L.Vogel, S.Mast, DamianGarcía Benito, RubénHusemann, BerndDannerbauer, H.Ellmeier, L.Cao, Y.GALAXIES: EVOLUTIONGALAXIES: KINEMATICS AND DYNAMICSGALAXIES: STAR FORMATIONGALAXIES: STRUCTUREISM: MOLECULEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a kpc-scale analysis of the relationship between the molecular depletion time (τdepmol ) and the orbital time (τorb) across the field of 39 face-on local galaxies, selected from the EDGE-CALIFA sample. We find that, on average, 5 per cent of the available molecular gas is converted into stars per orbital time, or τ depmol ~ 20 τorb. The resolved relation shows a scatter of ~0.5 dex. The scatter is ascribable to galaxies of different morphologies that follow different τ depmol -τorb relations which decrease in steepness from early- to late types. The morphologies appear to be linked with the star formation rate surface density, the molecular depletion time, and the orbital time, but they do not correlate with the molecular gas content of the galaxies in our sample.We speculate that in our molecular gas rich, early-type galaxies, the morphological quenching (in particular the disc stabilization via shear), rather than the absence of molecular gas, is the main factor responsible for their current inefficient star formation.Fil: Colombo, D.. Max Planck Institut Fur Astronomie; AlemaniaFil: Kalinova, V.. Max Planck Institut Fur Astronomie; AlemaniaFil: Utomo, D.. University Of California At Los Angeles. Department Of Physics And Astronomy.; Estados Unidos. Ohio State University; Estados UnidosFil: Rosolowsky, E.. University of Alberta; CanadáFil: Bolatto, A. D.. University of Maryland; Estados UnidosFil: Levy, R. C.. University of Maryland; Estados UnidosFil: Wong, T.. Southern Illinois University. Department Of Physics; Estados UnidosFil: Sanchez, S. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; MéxicoFil: Leroy, A. K.. Ohio University; Estados UnidosFil: Ostriker, E.. University of Princeton; Estados UnidosFil: Blitz, L.. Berkeley University; Estados UnidosFil: Vogel, S.. University of Maryland; Estados UnidosFil: Mast, Damian. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: García Benito, Rubén. Instituto de Astrofísica de Andalucía; EspañaFil: Husemann, Bernd. Max Planck Institut Fur Astronomie; AlemaniaFil: Dannerbauer, H.. Universidad de La Laguna; EspañaFil: Ellmeier, L.. Vienna University of Technology; AustriaFil: Cao, Y.. University of Illinois; Estados UnidosWiley Blackwell Publishing, Inc2018-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/134608Colombo, D.; Kalinova, V.; Utomo, D.; Rosolowsky, E.; Bolatto, A. D.; et al.; The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 475; 2; 4-2018; 1791-18080035-87111365-2966CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://academic.oup.com/mnras/article/475/2/1791/4743749info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx3233info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:24:31Zoai:ri.conicet.gov.ar:11336/134608instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:24:32.236CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence
title The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence
spellingShingle The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence
Colombo, D.
GALAXIES: EVOLUTION
GALAXIES: KINEMATICS AND DYNAMICS
GALAXIES: STAR FORMATION
GALAXIES: STRUCTURE
ISM: MOLECULES
title_short The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence
title_full The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence
title_fullStr The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence
title_full_unstemmed The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence
title_sort The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence
dc.creator.none.fl_str_mv Colombo, D.
Kalinova, V.
Utomo, D.
Rosolowsky, E.
Bolatto, A. D.
Levy, R. C.
Wong, T.
Sanchez, S. F.
Leroy, A. K.
Ostriker, E.
Blitz, L.
Vogel, S.
Mast, Damian
García Benito, Rubén
Husemann, Bernd
Dannerbauer, H.
Ellmeier, L.
Cao, Y.
author Colombo, D.
author_facet Colombo, D.
Kalinova, V.
Utomo, D.
Rosolowsky, E.
Bolatto, A. D.
Levy, R. C.
Wong, T.
Sanchez, S. F.
Leroy, A. K.
Ostriker, E.
Blitz, L.
Vogel, S.
Mast, Damian
García Benito, Rubén
Husemann, Bernd
Dannerbauer, H.
Ellmeier, L.
Cao, Y.
author_role author
author2 Kalinova, V.
Utomo, D.
Rosolowsky, E.
Bolatto, A. D.
Levy, R. C.
Wong, T.
Sanchez, S. F.
Leroy, A. K.
Ostriker, E.
Blitz, L.
Vogel, S.
Mast, Damian
García Benito, Rubén
Husemann, Bernd
Dannerbauer, H.
Ellmeier, L.
Cao, Y.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv GALAXIES: EVOLUTION
GALAXIES: KINEMATICS AND DYNAMICS
GALAXIES: STAR FORMATION
GALAXIES: STRUCTURE
ISM: MOLECULES
topic GALAXIES: EVOLUTION
GALAXIES: KINEMATICS AND DYNAMICS
GALAXIES: STAR FORMATION
GALAXIES: STRUCTURE
ISM: MOLECULES
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present a kpc-scale analysis of the relationship between the molecular depletion time (τdepmol ) and the orbital time (τorb) across the field of 39 face-on local galaxies, selected from the EDGE-CALIFA sample. We find that, on average, 5 per cent of the available molecular gas is converted into stars per orbital time, or τ depmol ~ 20 τorb. The resolved relation shows a scatter of ~0.5 dex. The scatter is ascribable to galaxies of different morphologies that follow different τ depmol -τorb relations which decrease in steepness from early- to late types. The morphologies appear to be linked with the star formation rate surface density, the molecular depletion time, and the orbital time, but they do not correlate with the molecular gas content of the galaxies in our sample.We speculate that in our molecular gas rich, early-type galaxies, the morphological quenching (in particular the disc stabilization via shear), rather than the absence of molecular gas, is the main factor responsible for their current inefficient star formation.
Fil: Colombo, D.. Max Planck Institut Fur Astronomie; Alemania
Fil: Kalinova, V.. Max Planck Institut Fur Astronomie; Alemania
Fil: Utomo, D.. University Of California At Los Angeles. Department Of Physics And Astronomy.; Estados Unidos. Ohio State University; Estados Unidos
Fil: Rosolowsky, E.. University of Alberta; Canadá
Fil: Bolatto, A. D.. University of Maryland; Estados Unidos
Fil: Levy, R. C.. University of Maryland; Estados Unidos
Fil: Wong, T.. Southern Illinois University. Department Of Physics; Estados Unidos
Fil: Sanchez, S. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; México
Fil: Leroy, A. K.. Ohio University; Estados Unidos
Fil: Ostriker, E.. University of Princeton; Estados Unidos
Fil: Blitz, L.. Berkeley University; Estados Unidos
Fil: Vogel, S.. University of Maryland; Estados Unidos
Fil: Mast, Damian. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: García Benito, Rubén. Instituto de Astrofísica de Andalucía; España
Fil: Husemann, Bernd. Max Planck Institut Fur Astronomie; Alemania
Fil: Dannerbauer, H.. Universidad de La Laguna; España
Fil: Ellmeier, L.. Vienna University of Technology; Austria
Fil: Cao, Y.. University of Illinois; Estados Unidos
description We present a kpc-scale analysis of the relationship between the molecular depletion time (τdepmol ) and the orbital time (τorb) across the field of 39 face-on local galaxies, selected from the EDGE-CALIFA sample. We find that, on average, 5 per cent of the available molecular gas is converted into stars per orbital time, or τ depmol ~ 20 τorb. The resolved relation shows a scatter of ~0.5 dex. The scatter is ascribable to galaxies of different morphologies that follow different τ depmol -τorb relations which decrease in steepness from early- to late types. The morphologies appear to be linked with the star formation rate surface density, the molecular depletion time, and the orbital time, but they do not correlate with the molecular gas content of the galaxies in our sample.We speculate that in our molecular gas rich, early-type galaxies, the morphological quenching (in particular the disc stabilization via shear), rather than the absence of molecular gas, is the main factor responsible for their current inefficient star formation.
publishDate 2018
dc.date.none.fl_str_mv 2018-04
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/134608
Colombo, D.; Kalinova, V.; Utomo, D.; Rosolowsky, E.; Bolatto, A. D.; et al.; The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 475; 2; 4-2018; 1791-1808
0035-8711
1365-2966
CONICET Digital
CONICET
url http://hdl.handle.net/11336/134608
identifier_str_mv Colombo, D.; Kalinova, V.; Utomo, D.; Rosolowsky, E.; Bolatto, A. D.; et al.; The EDGE-CALIFA survey: The influence of galactic rotation on the molecular depletion time across the Hubble sequence; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 475; 2; 4-2018; 1791-1808
0035-8711
1365-2966
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://academic.oup.com/mnras/article/475/2/1791/4743749
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx3233
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 12.982451

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