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Reconstructing the assembly of the baryonic mass in the hydra i cluster (Abell 1060) core using a multi dimensional space, from deep photometry and spectroscopic observations

Grant number: 12/22676-3
Support type:Scholarships abroad - Research Internship - Doctorate
Effective date (Start): March 01, 2013
Effective date (End): February 28, 2014
Field of knowledge:Physical Sciences and Mathematics - Astronomy
Principal Investigator:Claudia Lucia Mendes de Oliveira
Grantee:Carlos Eduardo Barbosa
Supervisor abroad: Magda Arnaboldi
Home Institution: Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG). Universidade de São Paulo (USP). São Paulo , SP, Brazil
Local de pesquisa : European Southern Observatory, La Serena (ESO), Chile  
Associated to the scholarship:11/21325-0 - Kinematics and stellar populations of nearby groups, BP.DR

Abstract

One of the major topics in Astronomy is the role of the environment on galactic properties, mainly due to our poor understanding of the physical mechanisms that act on the baryonic gas of galaxies. In this project, we plan to shed light on the subject by studying the core of the galaxy cluster Hydra I, combining deep photometry from VLT/FORS1 with high signal-to-noise multi-slit spectra from VLT/FORS2. For this purpose, we shall map the kinematics of the core producing a densely spaced grid covering the galaxy NGC3311 plus two detected dwarf systems and their surroundings. We also plan to determine the stellar populations of the same region to map the distribution of [alpha]/Fe and metallicity using Lick indexes. These products will be used jointly with published photometric data to the study of the current status of the system and its recent history of interaction with the intra-cluster medium. (AU)

Scientific publications
(References retrieved automatically from Web of Science and SciELO through information on FAPESP grants and their corresponding numbers as mentioned in the publications by the authors)
HILKER, M.; RICHTLER, T.; BARBOSA, C. E.; ARNABOLDI, M.; COCCATO, L.; DE OLIVEIRA, C. MENDES. The Hydra I cluster core II. Kinematic complexity in a rising velocity dispersion profile around the cD galaxy NGC3311. Astronomy & Astrophysics, v. 619, NOV 13 2018. Web of Science Citations: 2.

Please report errors in scientific publications list by writing to: cdi@fapesp.br.