Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage
- Autores
- Barrera-Ballesteros, J.K.; Garciá-Lorenzo, B.; Falcón-Barroso, J.; Van De Ven, G.; Lyubenova, M.; Wild, V.; Méndez-Abreu, J.; Sánchez, S. F.; Marquez, I.; Masegosa, J.; Monreal-Ibero, A.; Ziegler, Katharina B.; Del Olmo, A.; Verdes-Montenegro, L.; Garciá-Benito, R.; Husemann, B.; Mast, Damian; Kehrig, C.; Iglesias-Paramo, J.; Marino, R.A.; Aguerri, J. A. L.; Walcher, C. J.; Vílchez, J. M.; Bomans, D. J.; Cortijo-Ferrero, C.; González Delgado, R. M.; Bland-Hawthorn, J.; McIntosh, D.H.; Bekeraite, S.
- Año de publicación
- 2015
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present spatially resolved stellar and/or ionized gas kinematic properties for a sample of 103 interacting galaxies, tracing all merger stages: close companions, pairs with morphological signatures of interaction, and coalesced merger remnants. In order to distinguish kinematic properties caused by a merger event from those driven by internal processes, we compare our galaxies with a control sample of 80 non-interacting galaxies. We measure for both the stellar and the ionized gas components the major (projected) kinematic position angles (PAkin, approaching and receding) directly from the velocity distributions with no assumptions on the internal motions. This method also allow us to derive the deviations of the kinematic PAs from a straight line (δPAkin). We find that around half of the interacting objects show morpho-kinematic PA misalignments that cannot be found in the control sample. In particular, we observe those misalignments in galaxies with morphological signatures of interaction. On the other hand, thelevel of alignment between the approaching and receding sides for both samples is similar, with most of the galaxies displaying small misalignments. Radial deviations of the kinematic PA orientation from a straight line in the stellar component measured by δPAkin are large for both samples. However, for a large fraction of interacting galaxies the ionized gas δPAkin is larger than the typical values derived from isolated galaxies (48%), indicating that this parameter is a good indicator to trace the impact of interaction and mergers in the internal motions of galaxies. By comparing the stellar and ionized gas kinematic PA, we find that 42% (28/66) of the interacting galaxies have misalignments larger than 16°, compared to 10% from the control sample. Our results show the impact of interactions in the motion of stellar and ionized gas as well as the wide the variety of their spatially resolved kinematic distributions. This study also provides a local Universe benchmark for kinematic studies in merging galaxies at high redshift.
Fil: Barrera-Ballesteros, J.K.. Instituto de Astrofísica de Canarias; España
Fil: Garciá-Lorenzo, B.. Instituto de Astrofísica de Canarias; España
Fil: Falcón-Barroso, J.. Instituto de Astrofísica de Canarias; España
Fil: Van De Ven, G.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania
Fil: Lyubenova, M.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania
Fil: Wild, V.. University Of Saint Andrews; Reino Unido
Fil: Méndez-Abreu, J.. Instituto de Astrofísica de Canarias; España
Fil: Sánchez, S. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; México
Fil: Marquez, I.. Instituto de Astrofísica de Andalucía; España
Fil: Masegosa, J.. Instituto de Astrofísica de Andalucía; España
Fil: Monreal-Ibero, A.. Instituto de Astrofísica de Andalucía; España
Fil: Ziegler, Katharina B.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania
Fil: Del Olmo, A.. Instituto de Astrofísica de Andalucía; España
Fil: Verdes-Montenegro, L.. Instituto de Astrofísica de Andalucía; España
Fil: Garciá-Benito, R.. Instituto de Astrofísica de Andalucía; España
Fil: Husemann, B.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania
Fil: Mast, Damian. Centro Brasileiro de Pesquisas Físicas; Brasil. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Fil: Kehrig, C.. Instituto de Astrofísica de Andalucía; España
Fil: Iglesias-Paramo, J.. Instituto de Astrofísica de Andalucía; España
Fil: Marino, R.A.. Universidad Autónoma de Madrid; España
Fil: Aguerri, J. A. L.. Instituto de Astrofísica de Canarias; España
Fil: Walcher, C. J.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania
Fil: Vílchez, J. M.. Instituto de Astrofísica de Andalucía; España
Fil: Bomans, D. J.. Astronomical Institute of the Ruhr-University Bochum; Alemania
Fil: Cortijo-Ferrero, C.. Instituto de Astrofísica de Andalucía; España
Fil: González Delgado, R. M.. Instituto de Astrofísica de Andalucía; España
Fil: Bland-Hawthorn, J.. University of Sydney. Sydney Institute for Astronomy; Australia
Fil: McIntosh, D.H.. University of Missouri-Kansas City; Estados Unidos
Fil: Bekeraite, S.. Leibniz-Institut für Astrophysik Potsdam; Alemania - Materia
-
GALAXIES:EVOLUTION
GALAXIES:INTERACTIONS
GALAXIES:KINEMATICS AND DYNAMICS
GALAXIES:STATISTICS - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/69747
Ver los metadatos del registro completo
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Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stageBarrera-Ballesteros, J.K.Garciá-Lorenzo, B.Falcón-Barroso, J.Van De Ven, G.Lyubenova, M.Wild, V.Méndez-Abreu, J.Sánchez, S. F.Marquez, I.Masegosa, J.Monreal-Ibero, A.Ziegler, Katharina B.Del Olmo, A.Verdes-Montenegro, L.Garciá-Benito, R.Husemann, B.Mast, DamianKehrig, C.Iglesias-Paramo, J.Marino, R.A.Aguerri, J. A. L.Walcher, C. J.Vílchez, J. M.Bomans, D. J.Cortijo-Ferrero, C.González Delgado, R. M.Bland-Hawthorn, J.McIntosh, D.H.Bekeraite, S.GALAXIES:EVOLUTIONGALAXIES:INTERACTIONSGALAXIES:KINEMATICS AND DYNAMICSGALAXIES:STATISTICShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present spatially resolved stellar and/or ionized gas kinematic properties for a sample of 103 interacting galaxies, tracing all merger stages: close companions, pairs with morphological signatures of interaction, and coalesced merger remnants. In order to distinguish kinematic properties caused by a merger event from those driven by internal processes, we compare our galaxies with a control sample of 80 non-interacting galaxies. We measure for both the stellar and the ionized gas components the major (projected) kinematic position angles (PAkin, approaching and receding) directly from the velocity distributions with no assumptions on the internal motions. This method also allow us to derive the deviations of the kinematic PAs from a straight line (δPAkin). We find that around half of the interacting objects show morpho-kinematic PA misalignments that cannot be found in the control sample. In particular, we observe those misalignments in galaxies with morphological signatures of interaction. On the other hand, thelevel of alignment between the approaching and receding sides for both samples is similar, with most of the galaxies displaying small misalignments. Radial deviations of the kinematic PA orientation from a straight line in the stellar component measured by δPAkin are large for both samples. However, for a large fraction of interacting galaxies the ionized gas δPAkin is larger than the typical values derived from isolated galaxies (48%), indicating that this parameter is a good indicator to trace the impact of interaction and mergers in the internal motions of galaxies. By comparing the stellar and ionized gas kinematic PA, we find that 42% (28/66) of the interacting galaxies have misalignments larger than 16°, compared to 10% from the control sample. Our results show the impact of interactions in the motion of stellar and ionized gas as well as the wide the variety of their spatially resolved kinematic distributions. This study also provides a local Universe benchmark for kinematic studies in merging galaxies at high redshift.Fil: Barrera-Ballesteros, J.K.. Instituto de Astrofísica de Canarias; EspañaFil: Garciá-Lorenzo, B.. Instituto de Astrofísica de Canarias; EspañaFil: Falcón-Barroso, J.. Instituto de Astrofísica de Canarias; EspañaFil: Van De Ven, G.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; AlemaniaFil: Lyubenova, M.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; AlemaniaFil: Wild, V.. University Of Saint Andrews; Reino UnidoFil: Méndez-Abreu, J.. Instituto de Astrofísica de Canarias; EspañaFil: Sánchez, S. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; MéxicoFil: Marquez, I.. Instituto de Astrofísica de Andalucía; EspañaFil: Masegosa, J.. Instituto de Astrofísica de Andalucía; EspañaFil: Monreal-Ibero, A.. Instituto de Astrofísica de Andalucía; EspañaFil: Ziegler, Katharina B.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; AlemaniaFil: Del Olmo, A.. Instituto de Astrofísica de Andalucía; EspañaFil: Verdes-Montenegro, L.. Instituto de Astrofísica de Andalucía; EspañaFil: Garciá-Benito, R.. Instituto de Astrofísica de Andalucía; EspañaFil: Husemann, B.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; AlemaniaFil: Mast, Damian. Centro Brasileiro de Pesquisas Físicas; Brasil. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; ArgentinaFil: Kehrig, C.. Instituto de Astrofísica de Andalucía; EspañaFil: Iglesias-Paramo, J.. Instituto de Astrofísica de Andalucía; EspañaFil: Marino, R.A.. Universidad Autónoma de Madrid; EspañaFil: Aguerri, J. A. L.. Instituto de Astrofísica de Canarias; EspañaFil: Walcher, C. J.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; AlemaniaFil: Vílchez, J. M.. Instituto de Astrofísica de Andalucía; EspañaFil: Bomans, D. J.. Astronomical Institute of the Ruhr-University Bochum; AlemaniaFil: Cortijo-Ferrero, C.. Instituto de Astrofísica de Andalucía; EspañaFil: González Delgado, R. M.. Instituto de Astrofísica de Andalucía; EspañaFil: Bland-Hawthorn, J.. University of Sydney. Sydney Institute for Astronomy; AustraliaFil: McIntosh, D.H.. University of Missouri-Kansas City; Estados UnidosFil: Bekeraite, S.. Leibniz-Institut für Astrophysik Potsdam; AlemaniaEDP Sciences2015-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/69747Barrera-Ballesteros, J.K.; Garciá-Lorenzo, B.; Falcón-Barroso, J.; Van De Ven, G.; Lyubenova, M.; et al.; Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage; EDP Sciences; Astronomy and Astrophysics; 582; 10-20150004-63611432-0746CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201424935info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2015/10/aa24935-14/aa24935-14.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-10T13:13:05Zoai:ri.conicet.gov.ar:11336/69747instacron: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:34982025-09-10 13:13:05.939CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage |
| title |
Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage |
| spellingShingle |
Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage Barrera-Ballesteros, J.K. GALAXIES:EVOLUTION GALAXIES:INTERACTIONS GALAXIES:KINEMATICS AND DYNAMICS GALAXIES:STATISTICS |
| title_short |
Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage |
| title_full |
Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage |
| title_fullStr |
Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage |
| title_full_unstemmed |
Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage |
| title_sort |
Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage |
| dc.creator.none.fl_str_mv |
Barrera-Ballesteros, J.K. Garciá-Lorenzo, B. Falcón-Barroso, J. Van De Ven, G. Lyubenova, M. Wild, V. Méndez-Abreu, J. Sánchez, S. F. Marquez, I. Masegosa, J. Monreal-Ibero, A. Ziegler, Katharina B. Del Olmo, A. Verdes-Montenegro, L. Garciá-Benito, R. Husemann, B. Mast, Damian Kehrig, C. Iglesias-Paramo, J. Marino, R.A. Aguerri, J. A. L. Walcher, C. J. Vílchez, J. M. Bomans, D. J. Cortijo-Ferrero, C. González Delgado, R. M. Bland-Hawthorn, J. McIntosh, D.H. Bekeraite, S. |
| author |
Barrera-Ballesteros, J.K. |
| author_facet |
Barrera-Ballesteros, J.K. Garciá-Lorenzo, B. Falcón-Barroso, J. Van De Ven, G. Lyubenova, M. Wild, V. Méndez-Abreu, J. Sánchez, S. F. Marquez, I. Masegosa, J. Monreal-Ibero, A. Ziegler, Katharina B. Del Olmo, A. Verdes-Montenegro, L. Garciá-Benito, R. Husemann, B. Mast, Damian Kehrig, C. Iglesias-Paramo, J. Marino, R.A. Aguerri, J. A. L. Walcher, C. J. Vílchez, J. M. Bomans, D. J. Cortijo-Ferrero, C. González Delgado, R. M. Bland-Hawthorn, J. McIntosh, D.H. Bekeraite, S. |
| author_role |
author |
| author2 |
Garciá-Lorenzo, B. Falcón-Barroso, J. Van De Ven, G. Lyubenova, M. Wild, V. Méndez-Abreu, J. Sánchez, S. F. Marquez, I. Masegosa, J. Monreal-Ibero, A. Ziegler, Katharina B. Del Olmo, A. Verdes-Montenegro, L. Garciá-Benito, R. Husemann, B. Mast, Damian Kehrig, C. Iglesias-Paramo, J. Marino, R.A. Aguerri, J. A. L. Walcher, C. J. Vílchez, J. M. Bomans, D. J. Cortijo-Ferrero, C. González Delgado, R. M. Bland-Hawthorn, J. McIntosh, D.H. Bekeraite, S. |
| 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 author author author author |
| dc.subject.none.fl_str_mv |
GALAXIES:EVOLUTION GALAXIES:INTERACTIONS GALAXIES:KINEMATICS AND DYNAMICS GALAXIES:STATISTICS |
| topic |
GALAXIES:EVOLUTION GALAXIES:INTERACTIONS GALAXIES:KINEMATICS AND DYNAMICS GALAXIES:STATISTICS |
| 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 spatially resolved stellar and/or ionized gas kinematic properties for a sample of 103 interacting galaxies, tracing all merger stages: close companions, pairs with morphological signatures of interaction, and coalesced merger remnants. In order to distinguish kinematic properties caused by a merger event from those driven by internal processes, we compare our galaxies with a control sample of 80 non-interacting galaxies. We measure for both the stellar and the ionized gas components the major (projected) kinematic position angles (PAkin, approaching and receding) directly from the velocity distributions with no assumptions on the internal motions. This method also allow us to derive the deviations of the kinematic PAs from a straight line (δPAkin). We find that around half of the interacting objects show morpho-kinematic PA misalignments that cannot be found in the control sample. In particular, we observe those misalignments in galaxies with morphological signatures of interaction. On the other hand, thelevel of alignment between the approaching and receding sides for both samples is similar, with most of the galaxies displaying small misalignments. Radial deviations of the kinematic PA orientation from a straight line in the stellar component measured by δPAkin are large for both samples. However, for a large fraction of interacting galaxies the ionized gas δPAkin is larger than the typical values derived from isolated galaxies (48%), indicating that this parameter is a good indicator to trace the impact of interaction and mergers in the internal motions of galaxies. By comparing the stellar and ionized gas kinematic PA, we find that 42% (28/66) of the interacting galaxies have misalignments larger than 16°, compared to 10% from the control sample. Our results show the impact of interactions in the motion of stellar and ionized gas as well as the wide the variety of their spatially resolved kinematic distributions. This study also provides a local Universe benchmark for kinematic studies in merging galaxies at high redshift. Fil: Barrera-Ballesteros, J.K.. Instituto de Astrofísica de Canarias; España Fil: Garciá-Lorenzo, B.. Instituto de Astrofísica de Canarias; España Fil: Falcón-Barroso, J.. Instituto de Astrofísica de Canarias; España Fil: Van De Ven, G.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania Fil: Lyubenova, M.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania Fil: Wild, V.. University Of Saint Andrews; Reino Unido Fil: Méndez-Abreu, J.. Instituto de Astrofísica de Canarias; España Fil: Sánchez, S. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; México Fil: Marquez, I.. Instituto de Astrofísica de Andalucía; España Fil: Masegosa, J.. Instituto de Astrofísica de Andalucía; España Fil: Monreal-Ibero, A.. Instituto de Astrofísica de Andalucía; España Fil: Ziegler, Katharina B.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania Fil: Del Olmo, A.. Instituto de Astrofísica de Andalucía; España Fil: Verdes-Montenegro, L.. Instituto de Astrofísica de Andalucía; España Fil: Garciá-Benito, R.. Instituto de Astrofísica de Andalucía; España Fil: Husemann, B.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania Fil: Mast, Damian. Centro Brasileiro de Pesquisas Físicas; Brasil. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina Fil: Kehrig, C.. Instituto de Astrofísica de Andalucía; España Fil: Iglesias-Paramo, J.. Instituto de Astrofísica de Andalucía; España Fil: Marino, R.A.. Universidad Autónoma de Madrid; España Fil: Aguerri, J. A. L.. Instituto de Astrofísica de Canarias; España Fil: Walcher, C. J.. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania Fil: Vílchez, J. M.. Instituto de Astrofísica de Andalucía; España Fil: Bomans, D. J.. Astronomical Institute of the Ruhr-University Bochum; Alemania Fil: Cortijo-Ferrero, C.. Instituto de Astrofísica de Andalucía; España Fil: González Delgado, R. M.. Instituto de Astrofísica de Andalucía; España Fil: Bland-Hawthorn, J.. University of Sydney. Sydney Institute for Astronomy; Australia Fil: McIntosh, D.H.. University of Missouri-Kansas City; Estados Unidos Fil: Bekeraite, S.. Leibniz-Institut für Astrophysik Potsdam; Alemania |
| description |
We present spatially resolved stellar and/or ionized gas kinematic properties for a sample of 103 interacting galaxies, tracing all merger stages: close companions, pairs with morphological signatures of interaction, and coalesced merger remnants. In order to distinguish kinematic properties caused by a merger event from those driven by internal processes, we compare our galaxies with a control sample of 80 non-interacting galaxies. We measure for both the stellar and the ionized gas components the major (projected) kinematic position angles (PAkin, approaching and receding) directly from the velocity distributions with no assumptions on the internal motions. This method also allow us to derive the deviations of the kinematic PAs from a straight line (δPAkin). We find that around half of the interacting objects show morpho-kinematic PA misalignments that cannot be found in the control sample. In particular, we observe those misalignments in galaxies with morphological signatures of interaction. On the other hand, thelevel of alignment between the approaching and receding sides for both samples is similar, with most of the galaxies displaying small misalignments. Radial deviations of the kinematic PA orientation from a straight line in the stellar component measured by δPAkin are large for both samples. However, for a large fraction of interacting galaxies the ionized gas δPAkin is larger than the typical values derived from isolated galaxies (48%), indicating that this parameter is a good indicator to trace the impact of interaction and mergers in the internal motions of galaxies. By comparing the stellar and ionized gas kinematic PA, we find that 42% (28/66) of the interacting galaxies have misalignments larger than 16°, compared to 10% from the control sample. Our results show the impact of interactions in the motion of stellar and ionized gas as well as the wide the variety of their spatially resolved kinematic distributions. This study also provides a local Universe benchmark for kinematic studies in merging galaxies at high redshift. |
| publishDate |
2015 |
| dc.date.none.fl_str_mv |
2015-10 |
| 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/11336/69747 Barrera-Ballesteros, J.K.; Garciá-Lorenzo, B.; Falcón-Barroso, J.; Van De Ven, G.; Lyubenova, M.; et al.; Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage; EDP Sciences; Astronomy and Astrophysics; 582; 10-2015 0004-6361 1432-0746 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/69747 |
| identifier_str_mv |
Barrera-Ballesteros, J.K.; Garciá-Lorenzo, B.; Falcón-Barroso, J.; Van De Ven, G.; Lyubenova, M.; et al.; Tracing kinematic (mis)alignments in CALIFA merging galaxies: Stellar and ionized gas kinematic orientations at every merger stage; EDP Sciences; Astronomy and Astrophysics; 582; 10-2015 0004-6361 1432-0746 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
| dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201424935 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2015/10/aa24935-14/aa24935-14.html |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf |
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EDP Sciences |
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EDP Sciences |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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