Young, metal-enriched cores in early-type dwarf galaxies in the Virgo cluster based on colour gradients

Bibcode
2017A&A...606A.135U
DOI
10.1051/0004-6361/201730897
Urich, L.; Lisker, Thorsten; Janz, Joachim; van de Ven, Glenn; Leaman, Ryan; Boselli, Alessandro; Paudel, Sanjaya; Sybilska, Agnieszka; Peletier, Reynier F.; den Brok, Mark; Hensler, Gerhard; Toloba, Elisa; Falcón-Barroso, J.; Niemi, Sami-Matias
Bibliographical reference

Astronomy and Astrophysics, Volume 606, id.A135, 12 pp.

Advertised on:
10
2017
Journal
Astronomy and Astrophysics
Number of authors
14
IAC number of authors
1
Citations
24
Refereed citations
22
Description
Early-type dwarf galaxies are not simply featureless, old objects, but were found to be much more diverse, hosting substructures and a variety of stellar population properties. To explore the stellar content of faint early-type galaxies, and to investigate in particular those with recent central star formation, we study colours and colour gradients within one effective radius in optical (g - r) and near-infrared (i - H) bands for 120 Virgo cluster early-type galaxies with - 19 mag
Related projects
Group members
Traces of Galaxy Formation: Stellar populations, Dynamics and Morphology
We are a large, diverse, and very active research group aiming to provide a comprehensive picture for the formation of galaxies in the Universe. Rooted in detailed stellar population analysis, we are constantly exploring and developing new tools and ideas to understand how galaxies came to be what we now observe.
Ignacio
Martín Navarro
In progress
Type
Refereed
Galaxies
Photometry

It may interest you

  • Refereed
    Characterisation at Cryogenic Temperatures of an Attenuator for an Application of Astrophysical Instrumentation with MKIDs
    The use of non-cryogenic certified commercial electronics for cryogenic applications may be attractive due to their cost and availability, but it also carries risks related to reliability, performance and thermal compatibility. The decision to use commercial components that are not certified for cryogenics instead of components specifically
    Rodríguez Ramos L.F. et al.

    Advertised on:

    12
    2024
  • Refereed
    CLASH-VLT: Galaxy cluster MACS J0329–0211 and its surroundings using galaxies as kinematic tracers
    Context. The study of substructure is an important step in determining how galaxy clusters form. Aims. We aim to gain new insights into the controversial dynamical status of MACS J0329–0211 (MACS0329), a massive cluster at z = 0.4503 ± 0.0003, through a new analysis using a large sample of member galaxies as kinematic tracers. Methods. Our analysis
    Girardi, M. et al.

    Advertised on:

    12
    2024
    Bibcode
    2024A&A...692A.175G
    Citations
    0
  • Refereed
    The CHEOPS view of the climate of WASP-3 b
    Context. Hot Jupiters are giant planets subject to intense stellar radiation. The physical and chemical properties of their atmosphere make them the most amenable targets for atmospheric characterization. Aims. In this paper we analyze the photometry collected during the secondary eclipses of the hot Jupiter WASP-3 b by CHEOPS, TESS, and Spitzer
    Scandariato, G. et al.

    Advertised on:

    12
    2024
    Bibcode
    2024A&A...692A.129S
    Citations
    0