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The AMIGA sample of isolated galaxies XIII. The HI content of an almost "nurture free" sample
| Indexado |
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| DOI | 10.1051/0004-6361/201731448 | ||||
| Año | 2018 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Conclusions. The HI scaling relations of the AMIGA sample define an up-to-date metric of the HI content of almost "nurture free" galaxies. These relations allow the expected HI mass, in the absence of interactions, of an individual galaxy to be predicted to within 0.25 dex (for typical measurement uncertainties). These relations are thus suitable for use as statistical measures of the impact of interactions on the neutral gas content of galaxies.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Jones, Michael G. | Hombre |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 2 | Espada, Daniel | Hombre |
Natl Astron Observ Japan - Japón
Grad Univ Adv Studies SOKENDAI - Japón National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón The Graduate University for Advanced Studies - Japón |
| 3 | Verdes-Montenegro, Lourdes | Mujer |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 4 | Huchtmeier, W. K. | - |
Max Planck Inst Radioastron - Alemania
Max Planck Institute for Radio Astronomy - Alemania |
| 5 | Lisenfeld, Ute | - |
UNIV GRANADA - España
Universidad de Granada - España |
| 6 | Leon, Stephane | - |
ESO - Chile
Atacama Large Millimeter-submillimeter Array - Chile |
| 7 | Sulentic, J. | Hombre |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 8 | Sabater, J. | Hombre |
UNIV EDINBURGH - Reino Unido
University of Edinburgh, Institute for Astronomy - Reino Unido |
| 9 | JONES, DAVID E. | Hombre |
SAMSI - Estados Unidos
Duke Univ - Estados Unidos Statistical and Applied Mathematical Sciences Institute, USA - Estados Unidos Duke University - Estados Unidos |
| 10 | Sanchez, S. | - |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 11 | Garrido, Julian | Hombre |
CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| Fuente |
|---|
| National Science Foundation |
| Spanish Ministerio de Economía y Competitividad |
| Ministerio de Economía y Competitividad |
| Science and Technology Facilities Council |
| National Aeronautics and Space Administration |
| UK STFC |
| Alfred P. Sloan Foundation |
| European Regional Development Funds (FEDER) |
| Junta de Andalucia (Spain) |
| US Department of Energy Office of Science |
| DGI |
| MINECO/FEDER, UE |
| Marie Curie International Fellowship within the 6th European Community Framework Programme |
| Agradecimiento |
|---|
| We thanks E. Battaner, J. Vilchez, E. Perez, and S. Verley for their useful comments, and to staff members of the different telescopes from which data are presented in this paper, especially to those where we have observed: Arecibo, Effelsberg, Nancay, and GBT. We also thank J. R. Fisher for his assistance in obtaining GBT spectra. M.G.J. and L.V.M. acknowledge support from the grant AYA2015-65973-C3-1-R (MINECO/FEDER, UE). D.E. was supported by a Marie Curie International Fellowship during this work (MOIF-CT-2006-40298) within the 6th European Community Framework Programme. This work is supported by DGI Grant AYA 2008-06181-C02 and the Junta de Andalucia (Spain) P08-FQM-4205. U.L. acknowledges support by the research projects AYA2014-53506-P from the Spanish Ministerio de Economia y Competitividad, from the European Regional Development Funds (FEDER) and the Junta de Andalucia (Spain) grants FQM108. J.S. is grateful for support from the UK STFC via grant ST/M001229/1. D.E.J. acknowledges support from the National Science Foundation under Grant DMS-1127914 to the Statistical and Applied Mathematical Sciences Institute. This work also received support from the Junta de Andalucia (Spain) grant TIC-114. 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. We also acknowledge the use of the HyperLeda database. This research has made use of the SDSS. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the US Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/ |
| M.G.J. and L.V.M. acknowledge support from the grant AYA2015-65973-C3-1-R (MINECO/FEDER, UE). D.E. was supported by a Marie Curie International Fellowship during this work (MOIFCT- 2006-40298) within the 6th European Community Framework Programme. This work is supported by DGI Grant AYA 2008-06181-C02 and the Junta de Andalucía (Spain) P08-FQM-4205. U.L. acknowledges support by the research projects AYA2014-53506-P from the Spanish Ministerio de Economía y Competitividad, from the European Regional Development Funds (FEDER)and the Junta de Andalucía (Spain) grants FQM108. J.S. is grateful for support from the UK STFC via grant ST/M001229/1. D.E.J. acknowledges support from the National Science Foundation under Grant DMS-1127914 to the Statistical and Applied Mathematical Sciences Institute. This work also received support from the Junta de Andalucía (Spain) grant TIC-114. 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. |
