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/

  • Coevolution of supermassive black holes and their host galaxies

    Accretion onto a supermassive black hole (BH) is the most viable explanation for the huge emitted luminosity in active galaxies. Nowadays a wealth of observations have shown the presence of a BH in many nearby inactive bulges, suggesting that all massive spheroids harbor a BH. Moreover, at low redshift, fundamental correlations have been found

    Kotilainen, J. K. et al.

    Advertised on:

    10
    2008
    Citations
    4
  • Coevolution of Supermassive Black Holes and Their Host Galaxies

    Accretion onto a black hole (BH) is the most viable explanation for the huge emitted power in active galaxies. A wealth of observations have shown the presence of a BH in many nearby inactive bulges, suggesting that all massive spheroids harbor a BH. At low redshift, fundamental correlations have been found between the BH mass and the luminosity

    Kotilainen, J. K. et al.

    Advertised on:

    10
    2007
    Citations
    1
  • Cold Dark Matter Cusps in Low Surface Brightness Galaxies by Means of Stellar Kinematics

    A sample of galaxies characterized by a low surface brightness disk has dynamically studied using, as tracer, the stellar component. The kinematical data, taken along the major and minor axis, extend well within the disk region. The stellar kinematics is more regular and symmetric than the ionized-gas kinematics. Moreover, when comparing the

    Pizzella, A. et al.

    Advertised on:

    10
    2008
    Citations
    0
  • Coma Morphology and Rotational Dynamics of Comet 103P/Hartley 2 during the DIXI Encounter

    The target of the NASA DIXI mission, comet 103P/Hartley 2 is in a non-principal-axis (NPA) rotational state that was observed to be varying with time. However, there is still no consensus on the specific NPA rotational state during the 103P/Hartley 2 encounter by DIXI. We analyze the continuum features observed in ground-based images bracketing the

    Samarasinha, Nalin H. et al.

    Advertised on:

    10
    2012
    Citations
    1
  • Coma Treasury Survey. Structural parameters (Hoyos+, 2011)

    The observations (program GO 10861) were taken between 2006 November and 2007 January with the HST/ACS camera (2x4096x2048 pixels, 0.05arcsec/pixel, 3-arcsec interchip gap). (1 data file).

    Hoyos, C. et al.

    Advertised on:

    10
    2011
    Citations
    0
  • Combining visible-to-near-infrared spectra and WISE data of Hildas and Jupiter Trojans: preliminary results

    The Hilda asteroid group and Jupiter Trojans (JTs) are populations of primitive minor bodies whose origins have not been conclusively determined. In the framework of the so-called Nice Model, they are icy bodies scattered from the Kuiper Belt in an early epoch of the Solar System (the Late Heavy Bombardment) and finally trapped in the stable

    Ali-Lagoa, V. et al.

    Advertised on:

    10
    2013
    Citations
    0