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
    Automatic classification of optical sources candidates to be in the post-AGB stage
    Not Available
    Suárez, O. et al.

    Advertised on:

    0
    2001
    Bibcode
    2001hsa..conf..229S
    Citations
    0
  • Non-refereed
    Asteroseismology in the Main Sequence: The δ Scuti Stars of Praesepe Cluster (CD-ROM Directory: contribs/hernand)
    Not Available
    Hernández, M. M. et al.

    Advertised on:

    0
    2001
    Bibcode
    2001ASPC..223.1426H
    Citations
    0
  • Non-refereed
    Anisotropy in the mid-IR emission of Seyfert galaxies
    Based on Mid and far-IR data of a complete set of Seyfert galaxies we analyse the Spectral Energy Distributions (SED) of these objects. These SEDs can be separated into three thermal emission components. This separation can be used to introduce some sort of spatial resolution in the inherently low resolution ISO data. It can also be applied as a
    Pérez Garcia, A. M. et al.

    Advertised on:

    0
    2001
    Bibcode
    2001qhte.conf..255P
    Citations
    0
  • Non-refereed
    An Iceberg Scenario for Late-Type Spiral Galaxy Bulges
    Fitting exponential profiles to the bulges of the early-type spiral galaxies from de Jong & van der Kruit (1994) under-estimates their sizes at the 2-3 sigma significance level. Allowing for the range of structural shapes which these bulges possess - through fitting an r1/n profile - the mean effective bulge radius to disk scale-length ratio, re/h
    Graham, A. W. et al.

    Advertised on:

    0
    2001
    Bibcode
    2001ASPC..230..103G
    Citations
    1
  • Non-refereed
    Advantages of NIR Multiobject Spectroscopy of z ˜ 1 Galaxies
    Galaxy redshift surveys from z ˜ 1 to z ˜ 4 providing thousands of identified objects are already available. Only for a small and selected sample of those galaxies, near-infrared (NIR) spectroscopy and emission line studies exist. This is mainly due to the time-consuming work of observing one object at a time. This will change with the advent of
    Domínguez-Tagle, Carlos et al.

    Advertised on:

    0
    2001
    Bibcode
    2001defi.conf..153D
    Citations
    0