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Star-formation histories of local luminous infrared galaxies

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dc.contributor.authorPereira Santaella, Miguel
dc.contributor.authorAlonso Herrero, Almudena
dc.contributor.authorColina, Luis
dc.contributor.authorMiralles Caballero, Daniel
dc.contributor.authorPérez González, Pablo Guillermo
dc.contributor.authorArribas, Santiago
dc.contributor.authorBellocchi, Enrica
dc.contributor.authorCazzoli, Sara
dc.contributor.authorDiaz Santos, Tanio
dc.contributor.authorPiqueras López, Javier
dc.date.accessioned2023-06-18T06:47:00Z
dc.date.available2023-06-18T06:47:00Z
dc.date.issued2015-05
dc.description© ESO 2015. We thank the anonymous referee for comments and suggestions. We also thank the Nordic Optical Telescope and Isaac Newton Group staff for their support during the observations. We acknowledge support from the Spanish Plan Nacional de Astronomía y Astrofísica through grants AYA2010-21161-C02-1, AYA2010-21887-C04-03, AYA2012-32295, AYA2012-31447, AYA2012-31277, and AYA2012-39408-C02-01. Based on observations made with the Nordic Optical Telescope, operated by the Nordic Optical Telescope Scientific Association at the Observatorio del Roque de los Muchachos, La Palma, Spain, of the Instituto de Astrofísica de Canarias. The data presented here were obtained in part with ALFOSC, which is provided by the Instituto de Astrofísica de Andalucía (IAA) under a joint agreement with the University of Copenhagen and NOTSA. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
dc.description.abstractWe present analysis of the integrated spectral energy distribution (SED) from the ultraviolet (UV) to the far-infrared and H alpha of a sample of 29 local systems and individual galaxies with infrared (IR) luminosities between 10^11 L_⨀and 10^11.8 L_⨀. We combined new narrow-band Hα + [NII] and broad-band g, r optical imaging taken with the Nordic Optical Telescope (NOT), with archival GALEX, 2MASS, Spitzer, and Herschel data. Their SEDs (photometry and integrated Hα flux) were fitted simultaneously with a modified version of the MAGPHYS code using stellar population synthesis models for the UV-near-IR range and thermal emission models for the IR emission taking the energy balance between the absorbed and re-emitted radiation into account. From the SED fits, we derive the star-formation histories (SFH) of these galaxies. For nearly half of them, the star-formation rate appears to be approximately constant during the last few Gyr. In the other half, the current star-formation rate seems to be enhanced by a factor of 3-20 with respect to what occurred ∼1 Gyr ago. Objects with constant SFH tend to be more massive than starbursts, and they are compatible with the expected properties of a main-sequence (M-S) galaxy. Likewise, the derived SFHs show that all our objects were M-S galaxies ∼1 Gyr ago with stellar masses between 10^10.1 and 10^11.5 M_⨀. We also derived the average extinction (A_v = 0.6-3 mag) and the polycyclic aromatic hydrocarbon luminosity to L_IR ratio (0.03-0.16) from our fits. We combined the A_v with the total IR and Hα luminosities into a diagram that can be used to identify objects with rapidly changing (increasing or decreasing) SFR during the past 100 Myr.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Economía y Competitividad (MINECO)
dc.description.sponsorshipPlan Nacional de Astronomía y Astrofísica, España
dc.description.sponsorshipNational Aeronautics and Space Administration (NASA), EE.UU.
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/33190
dc.identifier.doi10.1051/0004-6361/201425359
dc.identifier.issn0004-6361
dc.identifier.officialurlhttp://dx.doi.org/10.1051/0004-6361/201425359
dc.identifier.relatedurlhttp://arxiv.org/abs/1502.07965
dc.identifier.relatedurlhttp://www.aanda.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/24162
dc.journal.titleAstronomy and astrophysics
dc.language.isoeng
dc.publisherEDP Sciencies
dc.relation.projectIDAYA2010-21161-C02-1
dc.relation.projectIDAYA2010-21887-C04-03
dc.relation.projectIDAYA2012-32295
dc.relation.projectIDAYA2012-31447
dc.relation.projectIDAYA2012-31277
dc.relation.projectIDAYA2012-39408-C02-01
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordIntegral field spectroscopy
dc.subject.keywordSpitzer-space-telescope
dc.subject.keywordEmission-line spectra
dc.subject.keywordForming galaxies
dc.subject.keywordOptical classification
dc.subject.keywordStellar populations
dc.subject.keywordMidinfrared spectroscopy
dc.subject.keywordInterstellar dust
dc.subject.keywordNearby galaxies
dc.subject.keywordFormation rates
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.titleStar-formation histories of local luminous infrared galaxies
dc.typejournal article
dc.volume.number577
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