Dataciencia

Colección SciELO Chile

Cluster galaxies in XMMU J2235-2557: galaxy population properties in most massive environments at z similar to 1.4

Indexado

WoS	WOS:000284625300071
Scopus	SCOPUS_ID:78649348250

DOI

10.1051/0004-6361/201015251

Año

2010

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

On the other hand, surface brightness distribution modeling of the massive red sequence galaxies may suggest that their size is often smaller than expected based on the local stellar mass vs. size relation. An evolution of the stellar mass vs. size relation might imply that, in spite of the overall early assembly of these sources, their evolution is not complete, and processes like minor (and likely dry) merging might still shape the structural properties of these objects to resemble those of their local counterparts, without substantially affecting their stellar mass or host stellar populations. Nonetheless, a definite conclusion on the actual relevance of size evolution for the studied early-type sample is precluded by possible systematics and biases.

Revista

Revista	ISSN
Astronomy & Astrophysics	1432-0746

Métricas Externas

PlumX	Altmetric	Dimensions

Muestra métricas de impacto externas asociadas a la publicación. Para mayor detalle:

Plumx: https://plumanalytics.com/learn/about-metrics/
Altmetric: https://www.altmetric.com/about-altmetrics/what-are-altmetrics/
Dimensions: https://www.dimensions.ai/why-dimensions/

Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

Muestra la distribución de disciplinas para esta publicación.

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

Colaboración Institucional

Muestra la distribución de colaboración, tanto nacional como extranjera, generada en esta publicación.

Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Strazzullo, Veronica	Mujer	Natl Radio Astron Observ - Estados Unidos National Radio Astronomy Observatory Socorro - Estados Unidos
2	Rosati, P.	Hombre	ESO - Alemania Observatorio Europeo Austral - Alemania
3	Pannella, M.	Hombre	Natl Radio Astron Observ - Estados Unidos National Radio Astronomy Observatory Socorro - Estados Unidos
4	Gobat, Raphael A. S.	Hombre	Univ Paris Diderot - Francia Commissariat a L'Energie Atomique CEA - Francia Commissariat a l'Energie Atomique et aux Energies Alternatives - Francia
5	SANTOS, JOANA S.	Mujer	Istituto Nazionale di Astrofisica - Italia Osservatorio Astronomico di Trieste - Italia
6	Nonino, M.	Hombre	Istituto Nazionale di Astrofisica - Italia Osservatorio Astronomico di Trieste - Italia
7	DEMARCO-BULL, RODRIGO ANDRES	Hombre	Universidad de Concepción - Chile
8	Lidman, Chris	Hombre	Australian Astron Observ - Australia Australian Astronomical Observatory - Australia
9	Tanaka, Masayuki	Hombre	ESO - Alemania Univ Tokyo - Japón Observatorio Europeo Austral - Alemania University of Tokyo - Japón The University of Tokyo - Japón
10	Mullis, C. R.	-	Wells Fargo Bank - Estados Unidos Wells Fargo Securities - Estados Unidos Wells Fargo - Estados Unidos
11	Núñez, C.	-	ESO - Alemania Observatorio Europeo Austral - Alemania
12	Rettura, Alessando	Hombre	Univ Calif Riverside - Estados Unidos University of California, Riverside - Estados Unidos
13	Jee, M. James	Hombre	UNIV CALIF DAVIS - Estados Unidos University of California, Davis - Estados Unidos
14	Bohringer, H.	Hombre	Max Planck Inst Extraterr Phys - Alemania Max Planck Institute for Extraterrestrial Physics - Alemania
15	Bender, R.	Hombre	Univ Sternwarte - Alemania Max Planck Inst Extraterr Phys - Alemania Max Planck Institute for Extraterrestrial Physics - Alemania Ludwig-Maximilians-Universität München - Alemania
16	Bouwens, Richard	Hombre	Leiden Univ - Países Bajos Univ Calif Santa Cruz - Estados Unidos Leiden Observatory Research Institute - Países Bajos University of California, Santa Cruz - Estados Unidos Sterrewacht Leiden - Países Bajos
17	Dawson, K. S.	Mujer	Univ Utah - Estados Unidos The University of Utah - Estados Unidos
18	Fassbender, R.	-	Max Planck Inst Extraterr Phys - Alemania Max Planck Institute for Extraterrestrial Physics - Alemania
19	Franx, Marijn	-	Leiden Univ - Países Bajos Leiden Observatory Research Institute - Países Bajos Sterrewacht Leiden - Países Bajos
20	Perlmutter, S.	Hombre	UNIV CALIF BERKELEY - Estados Unidos Lawrence Berkeley National Laboratory - Estados Unidos
21	Postman, M.	Hombre	Space Telescope Sci Inst - Estados Unidos STScI - Estados Unidos Space Telescope Science Institute - Estados Unidos

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Origen de Citas Identificadas

Muestra la distribución de países cuyos autores citan a la publicación consultada.

Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 27.4 %
Citas No-identificadas: 72.6 %

Muestra la distribución de instituciones nacionales o extranjeras cuyos autores citan a la publicación consultada.

Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 27.4 %
Citas No-identificadas: 72.6 %

Financiamiento

Fuente
DFG
NASA
ESO
Alexander von Humboldt Foundation
Ministerio de Ciencia e InnovaciÃ³n
Space Telescope Science Institute
Max-Planck Society
Universidad Complutense de Madrid
Office of Science, Office of High Energy and Nuclear Physics, of the US Department of Energy
NASA through Jet Propulsion Laboratory

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
We are grateful to T. Kodama for providing us with results from his elliptical galaxy evolution models. We thank the anonymous referee for a constructive report which helped us to improve the presentation of this work. V.S. acknowledges support under the ESO visitor program in Garching during the completion of this work. V.S. and M.P. acknowledge support from the Max-Planck Society and the Alexander von Humboldt Foundation, and from NASA through Jet Propulsion Laboratory contract No. 1289215. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. P.R. acknowledges support by the DFG cluster of excellence Origin and Structure of the Universe. Financial support for this work was partly provided by NASA through program GO-10496 from the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS 5-26555. This work was also supported inapart by the Director, Office of Science, Office of High Energy and Nuclear Physics, of the US Department of Energy under Contract No. AC02-05CH11231.
Partially supported by Project MTM2012-31298, MICINN and GR58/08 Grupo 920894, UCM, Spain.

Agradecimiento

We are grateful to T. Kodama for providing us with results from his elliptical galaxy evolution models. We thank the anonymous referee for a constructive report which helped us to improve the presentation of this work. V.S. acknowledges support under the ESO visitor program in Garching during the completion of this work. V.S. and M.P. acknowledge support from the Max-Planck Society and the Alexander von Humboldt Foundation, and from NASA through Jet Propulsion Laboratory contract No. 1289215. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. P.R. acknowledges support by the DFG cluster of excellence Origin and Structure of the Universe. Financial support for this work was partly provided by NASA through program GO-10496 from the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS 5-26555. This work was also supported inapart by the Director, Office of Science, Office of High Energy and Nuclear Physics, of the US Department of Energy under Contract No. AC02-05CH11231.

Partially supported by Project MTM2012-31298, MICINN and GR58/08 Grupo 920894, UCM, Spain.