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/

  • CO /J = 2-1/ observations of southern H II regions
    Maps in the CO (J = 2-1) line of the southern H II region complexes Carina Nebula and G333.6-0.2/RCW 106 are presented and discussed. Results for the Carina Nebula indicate a complicated spatial structure; an extended molecular cloud appears to be wrapped partly around the brightest parts of the H II region (Car I and Car II). The situation in
    de Graauw, T. et al.

    Advertised on:

    10
    1981
    Citations
    62
  • 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