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
    Investigating the dusty torus of Seyfert galaxies using SOFIA/FORCAST photometry
    We present 31.5 μm imaging photometry of 11 nearby Seyfert galaxies observed from the Stratospheric Observatory For Infrared Astronomy (SOFIA) using the Faint Object infraRed CAmera for the SOFIA Telescope (FORCAST). We tentatively detect extended 31 μm emission for the first time in our sample. In combination with this new data set, subarcsecond
    Fuller, L. et al.

    Advertised on:

    11
    2016
    Bibcode
    2016MNRAS.462.2618F
    Citations
    24
  • Non-refereed
    IPHASX J052531.2+281946: a new Planetary Nebula towards the Galactic Anticentre
    A planetary nebula has been discovered in the course of the INT/WFC Photometric Hα Survey (IPHAS) of the northern galactic plane. It is located near the galactic anticentre direction. Its small diameter and low Hβ brightness point to an extremely large distance. The ``Shklovskii'' galactocentric distance of DGC = 14-->20 kpc3 makes this nebula one
    Mampaso, A. et al.

    Advertised on:

    11
    2005
    Bibcode
    2005AIPC..804...14M
    Citations
    4
  • Non-refereed
    IR images of N159 in the LMC.
    The authors obtained near infrared images in J, H, and K filters of the H II region N159 in the LMC with the IR Imager on the 1.5 m telescope of CTIO. Some 50 sources are detected in an area of roughly 10 arc min squared. The region seems to be a site of active star formation associated to a large molecular complex and possibly coincides with one
    Rubio, M. et al.

    Advertised on:

    11
    1990
    Bibcode
    1990RMxAA..21..249R
    Citations
    1
  • Non-refereed
    IR light curves of four new low-mass eclipsing binaries
    In the last decade a significant amount of observational effort has been made to determine the physical parameters of low mass stars (M 1 Msol). The most recent observations appear to show a discrepancy between the mass-radius relation predicted by the models and that obtained from the observational data. This discrepancy appear to be explained by
    Iglesias Marzoa, R. et al.

    Advertised on:

    11
    2011
    Bibcode
    2011hsa6.conf..533I
    Citations
    0