Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Non-refereed
    Reconstructing Galactic Star Formation Histories from Star Cluster Age- and Mass-Distributions
    Observations show a relation between the brightest young star cluster and the present overall star formation rate of a galaxy. A possible explanation would be the formation of complete cluster populations in rather short formation epochs lasting ≈ 10 Myr. This implies that the star formation history of a galaxy is a sequence of formation epochs, in
    Maschberger, Th. et al.

    Advertised on:

    6
    2008
    Bibcode
    2008ASPC..388..409M
    Citations
    0
  • Non-refereed
    Recent Star Formation in Nearby Early-type Galaxies
    Motivated by recent progress in the study of early-type galaxies owing to technological advances, the launch of new space telescopes, and large ground-based surveys, we attempt a short review of our current understanding of the recent star formation activity in such intriguing galactic systems.
    Sarzi, M. et al.

    Advertised on:

    6
    2008
    Bibcode
    2008ASPC..390..218S
    Citations
    8
  • Refereed
    Properties of the Dwarf Galaxy Population in Galaxy Clusters
    We present the observational properties of the dwarf galaxy population (Mr>M*r+1) corresponding to one of the largest samples of spectroscopically confirmed nearby galaxy cluster members reported in the literature. We have observed that red dwarf galaxies (u-r>2.22) share the same cluster environment as the brightest cluster members (Mr
    Sánchez-Janssen, R. et al.

    Advertised on:

    6
    2008
    Bibcode
    2008ApJ...679L..77S
    Citations
    31
  • Non-refereed
    Preliminary results on the determination of the theoretical non-adiabatic observable phase lag (ψT) using VIRGO color photometry
    The helioseismic instruments aboard the SOHO satellite make it possible to measure solar oscillations as variations of the irradiance (VIRGO) or as variations of the photospheric velocity (GOLF). Theoretically, phase differences between different photometric bands are expected to be around 0 degrees over the p-mode frequency range. By using VIRGO
    Simoniello, R. et al.

    Advertised on:

    6
    2008
    Bibcode
    2008AN....329..498S
    Citations
    3