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
    EXPORT: Near-IR observations of Vega-type and pre-main sequence stars
    We present near-IR JHK photometric data of a sample of 58 main-sequence, mainly Vega-type, and pre-main sequence stars. The data were taken during four observing runs in the period May 1998 to January 1999 and form part of a coordinated effort with simultaneous optical spectroscopy and photo-polarimetry. The near-IR colors of the MS stars
    Eiroa, C. et al.

    Advertised on:

    1
    2001
    Bibcode
    2001A&A...365..110E
    Citations
    51
  • Non-refereed
    Comparison of parameters of low l solar p-modes at maximum and minimum activity
    Velocity measurements of disk integrated sunlight obtained by GOLF experiment aboard SOHO are used to find the parameters of solar p-modes (l
    Vázquez Ramió, Héctor et al.

    Advertised on:

    1
    2001
    Bibcode
    2001ESASP.464..555V
    Citations
    0
  • Non-refereed
    Circumnuclear dynamics in Mrk 273 and Mrk 231
    Mrk 273 and Mrk 231 are ultra-luminous IR galaxies which show signs of merger activity. Their radio continuum, HI and OH maser emission has been imaged on scales of tens of parsec using MERLIN. Mrk 273 and Mrk 231 are classed as Sy 2 and Sy 1 respectively. The distribution of material and velocity gradients shown by OH masers and HI absorption are
    Richards, A. M. S. et al.

    Advertised on:

    1
    2001
    Bibcode
    2001IAUS..205..212R
    Citations
    2
  • Non-refereed
    Chandra observations of M31
    As part of the Chandra Guaranteed Time Program we are imaging M31 once/month. The HRC is used to observe the entire galaxy to 10**37 ergs/sec, and interesting transients are followup up with ACIS observations which reach 10**36 ergs/sec. Thus the known (Galactic) types of accretion powered x-ray transients can detected and their spectra can be
    Garcia, M. R. et al.

    Advertised on:

    1
    2001
    Bibcode
    2001IAUS..205...38G
    Citations
    7