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
    Optical studies of V404 Cyg, the X-ray transient GS 2023+338. IV. The rotation speed of the companion star.
    Not Available
    Casares, J. et al.

    Advertised on:

    11
    1994
    Bibcode
    1994MNRAS.271L...5C
    Citations
    118
  • Refereed
    Optical variability of the ultracool dwarf TVLM 513-46546: evidence for inhomogeneous dust clouds
    We present multicolour photometry of the M8.5V ultracool dwarf `pulsar' TVLM 513-46546 (hereafter TVLM 513) obtained with the triple-beam photometer ULTRACAM. Data were obtained simultaneously in the Sloan-g' and Sloan-i' bands. The previously reported sinusoidal variability, with a period of 2 h, is recovered here. However, the Sloan-g' and Sloan
    Littlefair, S. P. et al.

    Advertised on:

    11
    2008
    Bibcode
    2008MNRAS.391L..88L
    Citations
    32
  • Refereed
    Orbital periods of cataclysmic variables identified by the SDSS. VI. The 4.5-h period eclipsing system SDSS J100658.40+233724.4
    We present time-resolved spectroscopy and photometry of SDSS J100658.40+233724.4, which we have discovered to be an eclipsing cataclysmic variable with an orbital period of 0.18591324 days (267.71507 min). The observed velocity amplitude of the secondary star is 276 ± 7 km s-1, which an irradiation correction reduces to 258 ± 12 km s-1. Doppler
    Southworth, J. et al.

    Advertised on:

    11
    2009
    Bibcode
    2009A&A...507..929S
    Citations
    29
  • Non-refereed
    Origin and fate of the most massive galaxies
    In the last five years there has been cumulative evidence showing that massivegalaxies have dramatically grown in size since z ˜ 3. This result hasremained very controversial as it seems at odd with our previous knowledgebased on the detailed analysis of the stellar populations of nearby massivegalaxies which shows that their stars were form very
    Trujillo, I.

    Advertised on:

    11
    2011
    Bibcode
    2011hsa6.conf..120T
    Citations
    0