The young population of the Local Group dwarf galaxy PHOENIX

Bibcode
1998mcdg.proc..271M
Martínez-Delgado, D.; Aparicio, A.
Bibliographical reference

The Magellanic Clouds and Other Dwarf Galaxies, Proceedings of the Bonn/Bochum-Graduiertenkolleg Workshop, held at the Physikzentrum Bad Honnef, Germany, January 19-22, 1998, Eds.: T. Richtler and J.M. Braun, Shaker Verlag, Aachen, ISBN 3-8265-4457-9, p. 271.

Advertised on:
12
1998
Number of authors
2
IAC number of authors
0
Citations
1
Refereed citations
1
Description
Not Available
Type
Non-refereed

It may interest you

  • Non-refereed
    3D scaling laws and projection effects in The300-NIKA2 Sunyaev-Zeldovich Large Program Twin Samples
    The abundance of galaxy clusters with mass and redshift is a wellknown cosmological probe. The cluster mass is a key parameter for studies that aim to constrain cosmological parameters using galaxy clusters, making it critical to understand and properly account for the errors in its estimates. Subsequently, it becomes important to correctly
    Paliwal, A. et al.

    Advertised on:

    6
    2024
    Bibcode
    2024EPJWC.29300037P
    Citations
    0
  • Non-refereed
    CONCERTO: Instrument and status
    CONCERTO (CarbON CII line in post-rEionization and ReionizaTiOn) is a low-resolution Fourier transform spectrometer dedicated to the study of star-forming galaxies and clusters of galaxies in the transparent millimeter windows from the ground. It is characterized by a wide instantaneous 18.6 arcmin field of view, operates at 130-310 GHz, and was
    Fasano, Alessandro et al.

    Advertised on:

    6
    2024
    Bibcode
    2024EPJWC.29300018F
    Citations
    0
  • Non-refereed
    Generating galaxy clusters mass density maps from mock multiview images via deep learning
    Galaxy clusters are composed of dark matter, gas and stars. Their dark matter component, which amounts to around 80% of the total mass, cannot be directly observed but traced by the distribution of diffused gas and galaxy members. In this work, we aim to infer the cluster's projected total mass distribution from mock observational data, i.e. stars
    de Andres, Daniel et al.

    Advertised on:

    6
    2024
    Bibcode
    2024EPJWC.29300013D
    Citations
    0
Go back