Stellar masses of star-forming galaxies at 0.3 < z < 1.2 in the GOYA survey

Bibcode
2005RMxAC..24..227C
Cristóbal-Hornillos, D.; Balcells, M.; Domínguez-Palmero, L.; Eliche-Moral, C.; Erwin, P.; Guzmán, R.; Prieto, M.
Bibliographical reference

II International GTC Workshop: Science with GTC 1st-light Instruments and the LMT (Eds. A. M. Hidalgo-Gámez, J. J. González, J. M. Rodríguez Espinosa, and S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 24, pp. 227-228 (2005) (http://www.astroscu.unam.mx/~rmaa/)

Advertised on:
12
2005
Number of authors
7
IAC number of authors
0
Citations
1
Refereed citations
1
Description
Starforming galaxies with compact morphology and high optical luminosity (LBCGs) are very common at redshitfs z = 0.4 - 1.2. Those galaxies are believed to have evolved more than other galaxy class during the last ~ 8 Gyr, and are a mayor contributor to the global star formation rate density of the universe at z ~ 1. A robust way to gauge their evolution is throught quantities that do not change much when the star formation activity ceases. In this poster we present the stellar mass measurements for a sample of 30 LBCGs from the GOYA photometric survey. The stellar masses are obtained by fitting the photometry in UBVIJK filters to a two component galaxy population model obtained with GISSELXXI.
Type
Non-refereed
Galaxies
Star formation

It may interest you

  • Non-refereed
    Massive characterisation of subgiants and red giants with TESS (Kepler and Gaia)
    TESS serves as a formidable tool for investigating stellar variability. Nonetheless, the adaptation of methodologies employed in other space missions, such as Kepler, to deduce long stellar rotation periods or solar-like stellar pulsations has been a challenge. The advent of multiple sectors of data for most stars every two years with the extended
    García, Rafael A. et al.

    Advertised on:

    9
    2024
    Bibcode
    2024tkas.confE.123G
    Citations
    0
  • Non-refereed
    Influence of the magnetic cycle on the excitation of solar-like acoustic modes
    The Sun's convective envelope generates, by dynamo effect, a surface magnetic field whose strength evolves on an 11-year cycle, with a change in polarity at the end of each cycle. Similar activity cycles exist in other solar-type stars, influencing the stars' dynamics, including the properties of acoustic oscillations, which are excited by
    Panetier, Eva et al.

    Advertised on:

    8
    2024
    Bibcode
    2024tkas.confE.107P
    Citations
    0
  • Non-refereed
    Twinkle, twinkle, undersampled star
    During the late subgiant/early giant stage, stars undergo fast evolutionary changes such as the readjustment of their internal rotation. It is of paramount importance to study this phase, in particular to understand the transport of angular momentum from the cores of stars to their envelopes. Bridging this knowledge gap is crucial to obtain more
    Liagre, Bastien et al.

    Advertised on:

    8
    2024
    Bibcode
    2024tkas.confE.101L
    Citations
    0