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The Fornax Deep Survey with the VST VII. Evolution and structure of late type galaxies inside the virial radius of the Fornax cluster
Indexado
WoS WOS:000476967300002
Scopus SCOPUS_ID:85069535835
DOI 10.1051/0004-6361/201935433
Año 2019
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



Conclusions. The main results of this work suggest that the disc-breaks of LTGs inside the virial radius of the Fornax cluster seem to have arisen through a variety of mechanisms (e.g. ram-pressure stripping, tidal disruption), which is evident in their outer-disc colours and the absence of molecular gas beyond their break radius in some cases. This can result in a variety of stellar populations inside and outside the break radii.

Revista



Revista ISSN
Astronomy & Astrophysics 0004-6361

Métricas Externas



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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Raj, M. A. Mujer Istituto Nazionale di Astrofisica - Italia
Univ Naples Federico II - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
Università Degli Studi di Napoli Federico II - Italia
2 Iodice, E. Mujer Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
3 Napolitano, N. Mujer Istituto Nazionale di Astrofisica - Italia
Sun Yat Sen Univ - China
Istituto Nazionale Di Astrofisica, Rome - Italia
Sun Yat-sen University Zhuhai Campus - China
Sun Yat-Sen University - China
4 Spavone, Marilena Mujer Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
5 Su, H-S. - Univ Oulu - Finlandia
Oulun Yliopisto - Finlandia
6 Peletier, R. E. Hombre Univ Groningen - Países Bajos
University of Groningen, Kapteyn Astronomical Institute - Países Bajos
Kapteyn Instituut - Países Bajos
7 Davis, Timothy A. Hombre Cardiff Univ - Reino Unido
Cardiff University - Reino Unido
8 Zabel, Nikki Mujer Cardiff Univ - Reino Unido
Cardiff University - Reino Unido
9 Hilker, Michael Hombre ESO - Alemania
10 Mieske, Steffen Hombre ESO - Chile
European Southern Observatory Santiago - Chile
11 Falcon-Barroso, Jesus Hombre Inst Astrofis Canarias - España
UNIV LA LAGUNA - España
Instituto Astrofisico de Canarias - España
Universidad de La Laguna - España
12 Cantiello, M. Mujer INAF Astron Abruzzo Observ - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
13 van de Ven, Glenn Hombre Univ Vienna - Austria
Universität Wien - Austria
14 Watkins, A. E. - Univ Oulu - Finlandia
Oulun Yliopisto - Finlandia
15 Salo, Heikki Hombre Univ Oulu - Finlandia
Oulun Yliopisto - Finlandia
16 Schipani, P. Hombre Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
17 Capaccioli, M. - Univ Naples Federico II - Italia
18 Venhola, Aku - Univ Groningen - Países Bajos
University of Groningen, Kapteyn Astronomical Institute - Países Bajos
Kapteyn Instituut - Países Bajos

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Financiamiento



Fuente
National Science Foundation
European Research Council
European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme
National Aeronautics and Space Administration
European Union’s Horizon 2020
VST project
H2020 Marie Skłodowska-Curie Actions
Horizon 2020
California Institute of Technology
Jet Propulsion Laboratory
Horizon 2020 Framework Programme
Sun Yat-sen University
European Union Horizon 2020
European Union Horizon 2020 Research and Innovation Programme under the Marie Sklodowska-Curie grant
NASA/IPAC
One hundred top talent program of Sun Yat-sen University
VST GTO programs
VST
Immune Tolerance Network
P.I. P.
H2020 Marie Skłodowska-Curie Actions
National Optical Astronomy Observatories
IPAC

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Agradecimientos



Agradecimiento
The authors are immensely grateful to the anonymous referee for the useful comments and suggestions that significantly improved this article. This publication has received funding from the European Union Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement n. 721463 to the SUNDIAL ITN network. This work is based on visitor mode observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under the following VST GTO programs: 094.B-0512(B), 094.B-0496(A), 096.B-0501(B), 096.B-0582(A). 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. E.I and M. S. acknowledge financial support from the VST project (P.I. P. Schipani). NRN acknowledges financial support from the "One hundred top talent program of Sun Yat-sen University"-grant N. 71000-18841229. GvdV acknowledges funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme under grant agreement No 724857 (Consolidator Grant ArcheoDyn). We thank Dr. Ignacio Trujillo and Dr. Johan Knapen for their suggestions and comments on the break radius of LTGs, and Dr. Crescenzo Tortora for his suggestions and comments. We would also like to show our gratitude to Dr. Tim de Zeeuw for his insights on this work.
Acknowledgements. The authors are immensely grateful to the anonymous referee for the useful comments and suggestions that significantly improved this article. This publication has received funding from the European Union Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement n. 721463 to the SUNDIAL ITN network. This work is based on visitor mode observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under the following VST GTO programs: 094.B-0512(B), 094.B-0496(A), 096.B-0501(B), 096.B-0582(A). 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. E.I and M. S. acknowledge financial support from the VST project (P.I. P. Schipani). NRN acknowledges financial support from the “One hundred top talent program of Sun Yat-sen University”-grant N. 71000-18841229. GvdV acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme under grant agreement No 724857 (Consolidator Grant ArcheoDyn). We thank Dr. Ignacio Trujillo and Dr. Johan Knapen for their suggestions and comments on the break radius of LTGs, and Dr. Crescenzo Tortora for his suggestions and comments. We would also like to show our gratitude to Dr. Tim de Zeeuw for his insights on this work.

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