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
    Resolving the Cosmic Infrared Background with ISOCAM
    The discovery in the COBE all-sky maps of a bright isotropic background in the far-IR/sub-mm, of likely extragalactic origin (CIRB), with a proeminent hump at a wavelength of 140 μm, has been interpreted at first as the integrated emission by dust present in very distant galaxies (Puget et al. 1996; Hauser et al. 1998). What is the relation between
    Cesarsky, Catherine et al.

    Advertised on:

    0
    2002
    Bibcode
    2002luml.conf..119C
    Citations
    0
  • Non-refereed
    Production of Li, Be and B in the Galaxy: cosmic ray processe in an interstellar environment
    Not Available
    Beckman, J. et al.

    Advertised on:

    0
    2002
    Bibcode
    2002MmSAI..73..994B
    Citations
    0
  • Non-refereed
    Polarización óptica de NGC 6231, evidencia de fenómenos energéticos
    In a typical young open cluster the polarimetric data shows, for normal stars, that the distribution of angles of the polarization vectors can be describe by a fixed value that caracterizes the cluster. Individual stars show some scatter over this mean angle because of fluctuations in the interstellar medium (ISM), variations in the magnetic field
    Feinstein, C. et al.

    Advertised on:

    0
    2002
    Bibcode
    2002BAAA...45...49F
    Citations
    0
  • Non-refereed
    Penetrating the Mask: All Spiral Galaxies become Barred on Bar Torque Scales between Zero and Six
    The Hubble classification scheme of galaxies is based on blue-light appearance. Atlases reveal the rich variety of responses of the Population I component (the "mask") of gas and dust to the underlying, older, stellar population. However, the Population I component may only constitute 5 percent of the dynamical mass of the galaxy; furthermore
    Block, D. L. et al.

    Advertised on:

    0
    2002
    Bibcode
    2002ASPC..273...97B
    Citations
    4