H II regions in the CALIFA survey: I. catalogue presentation
We present a new catalogue of H ii regions based on the integral field spectroscopy (IFS) data of the extended CALIFA and PISCO samples. The selection of H ii regions was based on two assumptions: a clumpy structure with high contrast of H α emission and an underlying stellar population comprising y...
| Autores: | , , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2020 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/213082 |
| Acceso en línea: | http://hdl.handle.net/10261/213082 |
| Access Level: | acceso abierto |
| Palabra clave: | Techniques: spectroscopic ISM: general HII regions Galaxies: ISM Galaxies: star formation |
| id |
ES_afb57fa005393a3dfb7ef62dda27c2f0 |
|---|---|
| oai_identifier_str |
oai:digital.csic.es:10261/213082 |
| network_acronym_str |
ES |
| network_name_str |
España |
| repository_id_str |
|
| spelling |
H II regions in the CALIFA survey: I. catalogue presentationEspinosa-Ponce, C.Sánchez, S. F.Morisset, C.Barrera-Ballesteros, Jorge K.Galbany, LluísGarcía-Benito, RubénLacerda, E.Mast, D.Techniques: spectroscopicISM: generalHII regionsGalaxies: ISMGalaxies: star formationWe present a new catalogue of H ii regions based on the integral field spectroscopy (IFS) data of the extended CALIFA and PISCO samples. The selection of H ii regions was based on two assumptions: a clumpy structure with high contrast of H α emission and an underlying stellar population comprising young stars. The catalogue provides the spectroscopic information of 26 408 individual regions corresponding to 924 galaxies, including the flux intensities and equivalent widths of 51 emission lines covering the wavelength range between 3745 and 7200 Å. To our knowledge, this is the largest catalogue of spectroscopic properties of H ii regions. We explore a new approach to decontaminate the emission lines from diffuse ionized gas contribution. This diffuse gas correction was estimated to correct every emission line within the considered spectral range. With the catalogue of H ii regions corrected, new demarcation lines are proposed for the classical diagnostic diagrams. Finally, we study the properties of the underlying stellar populations of the H ii regions. It was found that there is a direct relationship between the ionization conditions on the nebulae and the properties of stellar populations besides the physicals condition on the ionized regions.© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical SocietyWe thank the referee for the helpful comments that have improved the quality of this article. We are grateful for the support of CONACYT grants CB-285080, FC-2016-01-1916, and CB2015-254132, and funding from the DGAPA/PAPIIT-IA101217, DGAPA/PAPIITIN100519, and DGAPA/PAPIIT-107215 (UNAM) projects. This study uses data provided by the CALIFA survey (http://ca lifa.caha.es/); it is based on observations collected at the Centro Astronomico Hispano Alem ´ an (CAHA) at Calar Alto, operated ´ jointly by the Max-Planck-Institut fur Astronomie and the Instituto ¨ de Astrof´ısica de Andaluc´ıa (CSIC). LG was funded by the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement no. 839090. This research makes use of python (http://www.python.org), of Matplotlib (a framework to the creation of scientific plots for Python; Hunter 2007), Astropy (a Python package for astronomy; Astropy Collaboration 2013; Price-Whelan et al. 2018), and SciPy (a Python-based ecosystem of open-source software for mathematics, science, and engineering; Jones et al. 2001).Peer reviewedOxford University PressConsejo Nacional de Ciencia y Tecnología (México)Universidad Nacional Autónoma de MéxicoEuropean CommissionConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202020202020info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/213082reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/EC/H2020/839090http://dx.doi.org/ 10.1093/mnras/staa782Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/2130822026-05-22T06:33:51Z |
| dc.title.none.fl_str_mv |
H II regions in the CALIFA survey: I. catalogue presentation |
| title |
H II regions in the CALIFA survey: I. catalogue presentation |
| spellingShingle |
H II regions in the CALIFA survey: I. catalogue presentation Espinosa-Ponce, C. Techniques: spectroscopic ISM: general HII regions Galaxies: ISM Galaxies: star formation |
| title_short |
H II regions in the CALIFA survey: I. catalogue presentation |
| title_full |
H II regions in the CALIFA survey: I. catalogue presentation |
| title_fullStr |
H II regions in the CALIFA survey: I. catalogue presentation |
| title_full_unstemmed |
H II regions in the CALIFA survey: I. catalogue presentation |
| title_sort |
H II regions in the CALIFA survey: I. catalogue presentation |
| dc.creator.none.fl_str_mv |
Espinosa-Ponce, C. Sánchez, S. F. Morisset, C. Barrera-Ballesteros, Jorge K. Galbany, Lluís García-Benito, Rubén Lacerda, E. Mast, D. |
| author |
Espinosa-Ponce, C. |
| author_facet |
Espinosa-Ponce, C. Sánchez, S. F. Morisset, C. Barrera-Ballesteros, Jorge K. Galbany, Lluís García-Benito, Rubén Lacerda, E. Mast, D. |
| author_role |
author |
| author2 |
Sánchez, S. F. Morisset, C. Barrera-Ballesteros, Jorge K. Galbany, Lluís García-Benito, Rubén Lacerda, E. Mast, D. |
| author2_role |
author author author author author author author |
| dc.contributor.none.fl_str_mv |
Consejo Nacional de Ciencia y Tecnología (México) Universidad Nacional Autónoma de México European Commission Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Techniques: spectroscopic ISM: general HII regions Galaxies: ISM Galaxies: star formation |
| topic |
Techniques: spectroscopic ISM: general HII regions Galaxies: ISM Galaxies: star formation |
| description |
We present a new catalogue of H ii regions based on the integral field spectroscopy (IFS) data of the extended CALIFA and PISCO samples. The selection of H ii regions was based on two assumptions: a clumpy structure with high contrast of H α emission and an underlying stellar population comprising young stars. The catalogue provides the spectroscopic information of 26 408 individual regions corresponding to 924 galaxies, including the flux intensities and equivalent widths of 51 emission lines covering the wavelength range between 3745 and 7200 Å. To our knowledge, this is the largest catalogue of spectroscopic properties of H ii regions. We explore a new approach to decontaminate the emission lines from diffuse ionized gas contribution. This diffuse gas correction was estimated to correct every emission line within the considered spectral range. With the catalogue of H ii regions corrected, new demarcation lines are proposed for the classical diagnostic diagrams. Finally, we study the properties of the underlying stellar populations of the H ii regions. It was found that there is a direct relationship between the ionization conditions on the nebulae and the properties of stellar populations besides the physicals condition on the ionized regions.© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society |
| publishDate |
2020 |
| dc.date.none.fl_str_mv |
2020 2020 2020 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10261/213082 |
| url |
http://hdl.handle.net/10261/213082 |
| dc.language.none.fl_str_mv |
Inglés |
| language_invalid_str_mv |
Inglés |
| dc.relation.none.fl_str_mv |
#PLACEHOLDER_PARENT_METADATA_VALUE# info:eu-repo/grantAgreement/EC/H2020/839090 http://dx.doi.org/ 10.1093/mnras/staa782 Sí |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess |
| eu_rights_str_mv |
openAccess |
| dc.publisher.none.fl_str_mv |
Oxford University Press |
| publisher.none.fl_str_mv |
Oxford University Press |
| dc.source.none.fl_str_mv |
reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
| instname_str |
Consejo Superior de Investigaciones Científicas (CSIC) |
| reponame_str |
DIGITAL.CSIC. Repositorio Institucional del CSIC |
| collection |
DIGITAL.CSIC. Repositorio Institucional del CSIC |
| repository.name.fl_str_mv |
|
| repository.mail.fl_str_mv |
|
| _version_ |
1869416707549822976 |
| score |
15,811543 |