Dataciencia

Colección SciELO Chile

Stellar population and kinematics of NGC 404

Indexado

WoS	WOS:000285581500020
Scopus	SCOPUS_ID:77951693235

DOI

10.1051/0004-6361/200913137

Año

2010

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. We conclude that NGC 404 had a spiral morphology about 1 Gyr ago and that one or many merger events has triggered a morphological transition. The interstellar medium in the galaxy has two components, the cold molecular gas is most probably a remnant from its past spiral incarnation and the outer neutral hydrogen layer that has probably been acquired in one of the latest mergers.

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	Bouchard, A.	-	UNIV CAPE TOWN - República de Sudáfrica UNIV LYON 1 - Francia Univ Lyon - Francia Observ Lyon - Francia Ctr Rech Astrophys Lyon - Francia CNRS - Francia University of Cape Town - República de Sudáfrica Université de Lyon - Francia Université Claude Bernard Lyon 1 - Francia
2	Prugniel, P.	-	UNIV LYON 1 - Francia Univ Lyon - Francia Observ Lyon - Francia Ctr Rech Astrophys Lyon - Francia CNRS - Francia Université de Lyon - Francia Université Claude Bernard Lyon 1 - Francia Centre de Recherche Astrophysique de Lyon - Francia
3	Koleva, M.	-	UNIV LYON 1 - Francia Univ Lyon - Francia Observ Lyon - Francia Ctr Rech Astrophys Lyon - Francia CNRS - Francia UNIV LA LAGUNA - España Inst Astrofis Canarias - España Université de Lyon - Francia Instituto Astrofisico de Canarias - España Universidad de La Laguna - España Université Claude Bernard Lyon 1 - Francia
4	Sharina, M.	Mujer	Russian Acad Sci - Rusia SAO Branch - Chile Special Astrophysical Observatory, Russian Academy of Sciences - Rusia Institute Isaac Newton - Chile

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Financiamiento

Fuente
Spanish Ministry of Science and Innovation
Russian Foundation for Basic Research
French CNRS
South African Square Kilometre Array project

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Agradecimientos

Agradecimiento
We are grateful to Francois Simien who contributed to the early phases of this project, to Dmitry Makarov for his help during data reduction, and to the anonymous referee for the useful comments. A. B. acknowledges financial support from the South African Square Kilometre Array Project. M. K. acknowledges support by the Programa Nacional de Astronomia y Astrofisica of the Spanish Ministry of Science and Innovation under grant AYA2007-67752-C03-01. M. S. is partially supported by Russian Foundation for Basic Research grant 08-02-00627. We thank the Programme National Galaxies, from the French CNRS, for granting the observation time, and the staff from the Observatoire de Haute-Provence for their support during the observations.

Agradecimiento

We are grateful to Francois Simien who contributed to the early phases of this project, to Dmitry Makarov for his help during data reduction, and to the anonymous referee for the useful comments. A. B. acknowledges financial support from the South African Square Kilometre Array Project. M. K. acknowledges support by the Programa Nacional de Astronomia y Astrofisica of the Spanish Ministry of Science and Innovation under grant AYA2007-67752-C03-01. M. S. is partially supported by Russian Foundation for Basic Research grant 08-02-00627. We thank the Programme National Galaxies, from the French CNRS, for granting the observation time, and the staff from the Observatoire de Haute-Provence for their support during the observations.