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/

  • Refereed
    Brown dwarfs and very low mass stars in the Praesepe open cluster: a dynamically unevolved mass function?
    Context. Determination of the mass functions of open clusters of different ages allows us to infer the efficiency with which brown dwarfs are evaporated from clusters to populate the field. Aims: In this paper we present the results of a photometric survey to identify low mass and brown dwarf members of the old open cluster Praesepe (age 590+150
    Boudreault, S. et al.

    Advertised on:

    2
    2010
    Bibcode
    2010A&A...510A..27B
    Citations
    29
  • Non-refereed
    Apparent Novae in M81: M81N 2010-01a and M81N 2010-01b
    CBET 2170 available at Central Bureau for Astronomical Telegrams.
    Hornoch, K. et al.

    Advertised on:

    2
    2010
    Bibcode
    2010CBET.2170....2H
    Citations
    0
  • Non-refereed
    Apparent Novae in M81: M81N 2010-01a and M81N 2010-01b
    CBET 2170 available at Central Bureau for Astronomical Telegrams.
    Hornoch, K. et al.

    Advertised on:

    2
    2010
    Bibcode
    2010CBET.2170....1H
    Citations
    1
  • Refereed
    An HST/WFPC2 survey of bright young clusters in M 31. IV. Age and mass estimates
    Aims: We present the main results of an imaging survey of possible young massive clusters (YMC) in M 31 performed with the Wide Field and Planetary Camera 2 (WFPC2) on the Hubble Space Telescope (HST), with the aim of estimating their age and their mass. We obtained shallow (to B ˜ 25) photometry of individual stars in 19 clusters (of the 20
    Perina, S. et al.

    Advertised on:

    2
    2010
    Bibcode
    2010A&A...511A..23P
    Citations
    29
  • Refereed
    A scenario of planet erosion by coronal radiation
    Context. According to theory, high-energy emission from the coronae of cool stars can severely erode the atmospheres of orbiting planets. No observational tests of the long-term erosion effects have been made yet. Aims: We analyze the current distribution of planetary mass with X-ray irradiation of the atmospheres to make an observational
    Sanz-Forcada, J. et al.

    Advertised on:

    2
    2010
    Bibcode
    2010A&A...511L...8S
    Citations
    74