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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/134608
Ver los metadatos del registro completo
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oai:ri.conicet.gov.ar:11336/134608 |
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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 Técnicas2025-09-29T09:55:25Zoai: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:34982025-09-29 09:55:25.392CONICET 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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1844613671321337856 |
score |
13.070432 |