Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey
We present IRAM-30 m Telescope 12CO and 13CO observations of a sample of 55 luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) in the local universe. This sample is a subset of the Great Observatory All-Sky LIRG Survey (GOALS), for which we use ancillary multi-wavelength data to better...
| Autores: | , , , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2019 |
| País: | España |
| Institución: | Universidad de Zaragoza |
| Repositorio: | Zaguán. Repositorio Digital de la Universidad de Zaragoza |
| OAI Identifier: | oai:zaguan.unizar.es:96040 |
| Acceso en línea: | http://zaguan.unizar.es/record/96040 |
| Access Level: | acceso abierto |
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Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG SurveyHerrero-Illana, R.Privon, G.C.Evans, A.S.Diaz-Santos, T.Perez-Torres, M.A.Alberdi, A.Iwasawa, K.Armus, L.Aalto, S.Mazzarella, J.Chu, J.Sanders, D.B.Barcos-Munoz, L.Charmandaris, V.Linden, S.T.Yoon, I.Frayer, D.T.Inami, H.Kim, D.C.Borish, H.J.Conway, J.Murphy, E.J.Song, Y.Stierwalt, S.Surace, J.We present IRAM-30 m Telescope 12CO and 13CO observations of a sample of 55 luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) in the local universe. This sample is a subset of the Great Observatory All-Sky LIRG Survey (GOALS), for which we use ancillary multi-wavelength data to better understand their interstellar medium and star formation properties. Fifty-three (96%) of the galaxies are detected in 12CO, and 29 (52%) are also detected in 13CO above a 3σ level. The median full width at zero intensity (FWZI) velocity of the CO line emission is 661 km s−1, and ∼54% of the galaxies show a multi-peak CO profile. Herschel photometric data is used to construct the far-IR spectral energy distribution of each galaxy, which are fit with a modified blackbody model that allows us to derive dust temperatures and masses, and infrared luminosities. We make the assumption that the gas-to-dust mass ratio of (U)LIRGs is comparable to local spiral galaxies with a similar stellar mass (i.e., gas/dust of mergers is comparable to their progenitors) to derive a CO-to-H2 conversion factor of ⟨α⟩ = 1.8−0.8+1.3 M⊙ (K km s−1 pc2)−1; such a value is comparable to that derived for (U)LIRGs based on dynamical mass arguments. We derive gas depletion times of 400 − 600 Myr for the (U)LIRGs, compared to the 1.3 Gyr for local spiral galaxies. Finally, we re-examine the relationship between the 12CO/13CO ratio and dust temperature, confirming a transition to elevated ratios in warmer systems.2019info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://zaguan.unizar.es/record/96040reponame:Zaguán. Repositorio Digital de la Universidad de Zaragozainstname:Universidad de ZaragozaInglésinfo:eu-repo/grantAgreement/ES/MINECO/AYA2012-38491-C02-02info:eu-repo/grantAgreement/ES/MINECO/AYA2015-63939-C2-1-Pinfo:eu-repo/semantics/openAccessoai:zaguan.unizar.es:960402026-05-29T13:59:51Z |
| dc.title.none.fl_str_mv |
Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey |
| title |
Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey |
| spellingShingle |
Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey Herrero-Illana, R. |
| title_short |
Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey |
| title_full |
Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey |
| title_fullStr |
Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey |
| title_full_unstemmed |
Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey |
| title_sort |
Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey |
| dc.creator.none.fl_str_mv |
Herrero-Illana, R. Privon, G.C. Evans, A.S. Diaz-Santos, T. Perez-Torres, M.A. Alberdi, A. Iwasawa, K. Armus, L. Aalto, S. Mazzarella, J. Chu, J. Sanders, D.B. Barcos-Munoz, L. Charmandaris, V. Linden, S.T. Yoon, I. Frayer, D.T. Inami, H. Kim, D.C. Borish, H.J. Conway, J. Murphy, E.J. Song, Y. Stierwalt, S. Surace, J. |
| author |
Herrero-Illana, R. |
| author_facet |
Herrero-Illana, R. Privon, G.C. Evans, A.S. Diaz-Santos, T. Perez-Torres, M.A. Alberdi, A. Iwasawa, K. Armus, L. Aalto, S. Mazzarella, J. Chu, J. Sanders, D.B. Barcos-Munoz, L. Charmandaris, V. Linden, S.T. Yoon, I. Frayer, D.T. Inami, H. Kim, D.C. Borish, H.J. Conway, J. Murphy, E.J. Song, Y. Stierwalt, S. Surace, J. |
| author_role |
author |
| author2 |
Privon, G.C. Evans, A.S. Diaz-Santos, T. Perez-Torres, M.A. Alberdi, A. Iwasawa, K. Armus, L. Aalto, S. Mazzarella, J. Chu, J. Sanders, D.B. Barcos-Munoz, L. Charmandaris, V. Linden, S.T. Yoon, I. Frayer, D.T. Inami, H. Kim, D.C. Borish, H.J. Conway, J. Murphy, E.J. Song, Y. Stierwalt, S. Surace, J. |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author |
| description |
We present IRAM-30 m Telescope 12CO and 13CO observations of a sample of 55 luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) in the local universe. This sample is a subset of the Great Observatory All-Sky LIRG Survey (GOALS), for which we use ancillary multi-wavelength data to better understand their interstellar medium and star formation properties. Fifty-three (96%) of the galaxies are detected in 12CO, and 29 (52%) are also detected in 13CO above a 3σ level. The median full width at zero intensity (FWZI) velocity of the CO line emission is 661 km s−1, and ∼54% of the galaxies show a multi-peak CO profile. Herschel photometric data is used to construct the far-IR spectral energy distribution of each galaxy, which are fit with a modified blackbody model that allows us to derive dust temperatures and masses, and infrared luminosities. We make the assumption that the gas-to-dust mass ratio of (U)LIRGs is comparable to local spiral galaxies with a similar stellar mass (i.e., gas/dust of mergers is comparable to their progenitors) to derive a CO-to-H2 conversion factor of ⟨α⟩ = 1.8−0.8+1.3 M⊙ (K km s−1 pc2)−1; such a value is comparable to that derived for (U)LIRGs based on dynamical mass arguments. We derive gas depletion times of 400 − 600 Myr for the (U)LIRGs, compared to the 1.3 Gyr for local spiral galaxies. Finally, we re-examine the relationship between the 12CO/13CO ratio and dust temperature, confirming a transition to elevated ratios in warmer systems. |
| publishDate |
2019 |
| dc.date.none.fl_str_mv |
2019 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion |
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article |
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publishedVersion |
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http://zaguan.unizar.es/record/96040 |
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http://zaguan.unizar.es/record/96040 |
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Inglés |
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Inglés |
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info:eu-repo/grantAgreement/ES/MINECO/AYA2012-38491-C02-02 info:eu-repo/grantAgreement/ES/MINECO/AYA2015-63939-C2-1-P |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
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reponame:Zaguán. Repositorio Digital de la Universidad de Zaragoza instname:Universidad de Zaragoza |
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Universidad de Zaragoza |
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Zaguán. Repositorio Digital de la Universidad de Zaragoza |
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