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/

  • The distances of the Galactic novae
    Utilizing the unique location of red clump giants on colour-magnitude diagrams obtained from various near-infrared surveys, we derived specific reddening-distance relations towards 119 Galactic novae for which independent reddening measurements are available. Using the derived distance-extinction relation and the independent measurements of
    Özdönmez, A. et al.

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    9
    2016
    Citations
    22
  • The double-mode nature of the HADS star GSC 00144-03031 and the Petersen diagram of the class
    The double-mode pulsation of GSC 00144-03031 has been detected when searching for COROT targets. A very large dataset composed of 4722 photometric measurements was collected at six observatories in Europe and America. There is no hint of the excitation of additional modes (down to 0.6 mmag) and therefore GSC 00144-03031 seems to be a pure double
    Poretti, E. et al.

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    9
    2005
    Citations
    69
  • The Dust Environment of Main-Belt Comet P/2010 R2 (La Sagra)
    We present a model of the dust environment of Main-Belt Comet P/2010 R2 (La Sagra) from images acquired during the period 2010 October-2011 January. The tails are best simulated by anisotropic ejection models, with emission concentrated near the nucleus south pole, the spin axis having an obliquity near 90°, indicative of a possible seasonally
    Moreno, F. et al.

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    9
    2011
    Citations
    41
  • The dynamical status of ZwCl 2341.1+0000: a very elongated galaxy structure with a complex radio emission
    We study the dynamical status of the galaxy system ZwCl 2341.1+0000, a filamentary multi-Mpc galaxy structure associated with a complex diffuse radio emission. Our analysis is mainly based on new spectroscopic data for 128 galaxies acquired at the Italian Telescopio Nazionale Galileo. We also use optical data available in the Sloan Digital Sky
    Boschin, W. et al.

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    9
    2013
    Citations
    21
  • The Dynamics of the Outer Regions of the Coma Cluster
    We apply the spherical infall model to compare the observed distribution of radial velocities of galaxies around Coma with predictions that are based on optical and X-ray overdensity profiles. Two optically selected galaxy catalogues, the CfA redshift survey and a UKST plate scanned with the APM, are used to determine the overdensity profile of the
    van Haarlem, M. P. et al.

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    9
    1993
    Citations
    36