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
    The Rotation of Comet 1995 O1 (Hale-Bopp) at Perihelion
    Narrow band near infrared images of comet 1995 O1 (Hale-Bopp), where obtained in day-time, during April 1997, using the 1.52m Carlos Sanchez Telescope, at Teide Observatory (Tenerife, Spain), by the Comet Hale Bopp European Team. The comet was observed continuously for up to 11 hours hours each day on a total of 15 days. This allows us to obtain a
    Kidger, M. et al.

    Advertised on:

    12
    1997
    Bibcode
    1997AAS...191.8801K
    Citations
    1
  • Refereed
    The rotation-metallicity relation for the Galactic disk as measured in the Gaia DR1 TGAS and APOGEE data
    Aims: Previous studies have found that the Galactic rotation velocity-metallicity (V-[Fe/H]) relations for the thin and thick disk populations show negative and positive slopes, respectively. The first Gaia data release includes the Tycho-Gaia Astrometric Solution (TGAS) information, which we use to analyze the V-[Fe/H] relation for a strictly
    Allende Prieto, C. et al.

    Advertised on:

    12
    2016
    Bibcode
    2016A&A...596A..98P
    Citations
    0
  • Refereed
    The rotation-metallicity relation for the Galactic disk as measured in the Gaia DR1 TGAS and APOGEE data
    Aims: Previous studies have found that the Galactic rotation velocity-metallicity (V-[Fe/H]) relations for the thin and thick disk populations show negative and positive slopes, respectively. The first Gaia data release includes the Tycho-Gaia Astrometric Solution (TGAS) information, which we use to analyze the V-[Fe/H] relation for a strictly
    Cropper, Mark et al.

    Advertised on:

    12
    2016
    Bibcode
    2016A&A...596A..98A
    Citations
    30
  • Refereed
    The Sagittarius dwarf irregular galaxy (SagDIG): distance and star formation history
    The distance, star formation history and global properties of the Local Group dIrr galaxy SagDIG are derived based on an [I-(V-I)] colour-magnitude diagram of ~ 1550 stars. A distance of 1.06+/- 0.10 Mpc is obtained from the I magnitude of the TRGB. This corresponds to 1.17 Mpc to the barycenter of the Local Group and 1.34 to M 31, being DDO 210
    Karachentsev, I. et al.

    Advertised on:

    12
    1999
    Bibcode
    1999A&A...352..363K
    Citations
    32
  • Refereed
    The SAURON project - VIII. OASIS/CFHT integral-field spectroscopy of elliptical and lenticular galaxy centres
    We present high spatial resolution integral-field spectroscopy of 28 elliptical (E) and lenticular (S0) galaxies from the SAURON representative survey obtained with the OASIS spectrograph during its operation at the Canada-France-Hawaii Telescope. These seeing-limited observations explore the central 8 × 10 arcsec2 (typically 1 kpc diameter)
    McDermid, Richard M. et al.

    Advertised on:

    12
    2006
    Bibcode
    2006MNRAS.373..906M
    Citations
    179
  • Non-refereed
    The SAURON View of the Nuclear Ring in M100
    Nuclear rings located within the central 1-2 kiloparsecs of barred spiral galaxies are often found to contain a large fraction of the total star formation taking place in a galaxy. Under the influence of a bar, gas can be channelled inwards along narrow ridges where shocks develop in the gas flow. We observe these shocks as dark dustlanes along the
    Allard, E. L. et al.

    Advertised on:

    12
    2005
    Bibcode
    2005INGN...10....8A
    Citations
    0