Zobrazeno 1 - 2
of 2
pro vyhledávání: '"Daniel Hernández Lang"'
Autor:
Antonela Monachesi, C. Lima-Dias, Daniel Hernández-Lang, Yara L. Jaffé, P. Dimauro, Ana L. Chies-Santos, Alberto Molino, Daniela Olave-Rojas, Paulo A. A. Lopes, T. Ribeiro, Carlos Eduardo Barbosa, L. Sampedro, F. R. Herpich, Alvaro Alvarez-Candal, Claudia Mendes de Oliveira, Arianna Cortesi, Eduardo Telles, Fabricio Ferrari, Diego Pallero, Antonio Kanaan, S. Torres-Flores, Ricardo Amorín, William Schoenell
Publikováno v:
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Universidad de Alicante (UA)
The nearby Hydra Cluster ($\sim$50 Mpc) is an ideal laboratory to understand, in detail, the influence of the environment on the morphology and quenching of galaxies in dense environments. We study the Hydra cluster galaxies in the inner regions ($1R
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ffd32d6d0e454790ed24554ae4325636
http://hdl.handle.net/10045/111713
http://hdl.handle.net/10045/111713
Autor:
Elizabeth Johana Gonzalez, L Héctor Cuevas, Martín de los Rios, Tania Aguirre Tagliaferro, J R Mariano Domínguez, G. A. Oio, José Luis Nilo Castellón, Carlos Valotto, Daniel Hernández Lang
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Merging galaxy clusters allow for the study of different mass components, dark and baryonic, separately. Also, their occurrence enables to test the ΛCDM scenario, which can be used to put constraints on the selfinteracting cross-section of the dark-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1cdfb2a1e83f6bf17c98f3d3a231637e
https://www.aanda.org/10.1051/0004-6361/201732003
https://www.aanda.org/10.1051/0004-6361/201732003