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 complex structure of HH 110 as revealed from Integral Field Spectroscopy
    HH 110 is a rather peculiar HerbigHaro object in Orion that originates due to the deflection of another jet (HH 270) by a dense molecular clump, instead of being directly ejected from a young stellar object. Here we present new results on the kinematics and physical conditions of HH 110 based on Integral Field Spectroscopy. The 3D spectral data
    López, R. et al.

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    8
    2010
    Citations
    5
  • The complexity of the coronal line region in AGNs: Gas-jet interactions and outflows revealed by NIR spectroscopy
    Apart from the classical broad line region (BLR) at small core distances, and the extended classical narrow-line region (NLR), a subset of active galactic nuclei (AGN) show, in their spectra, lines from very highly ionised atoms, known as Coronal lines (CLs). The precise nature and origin of these CLs remain uncertain. Advances on this matter
    Rodríguez-Ardila, A. et al.

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    8
    2016
    Citations
    0
  • The control unit of the near infrared spectrograph of the EUCLID space mission: preliminary design
    The Near Infrared Spectrograph and Photometer (NISP) is one of the instruments on board the ESA EUCLID mission. The Universidad Politecnica de Cartagena and Instituto de Astrofisica de Canarias are responsible of the Instrument Control Unit of the NISP (NI-ICU) in the Euclid Consortium. The NI-ICU main functions are: communication with the S/C and
    Toledo-Moreo, R. et al.

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    8
    2014
    Citations
    1
  • The cool ZZ Ceti star PG 2303+243: observations and analysis of variability in 2004
    PG 2303+243 is a cool DA variable (also called ZZ Ceti) star with a rich pulsation spectrum and variable amplitudes. A mini-campaign involving six observatories yielded time-resolved photometric measurements of PG 2303+243 during the period 2004 September 5-20. A duty cycle of 35 per cent was achieved. We detected 24 possible independent
    Pakštienė, E. et al.

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    8
    2011
    Citations
    6
  • The core-halo structure of IC 418
    Deep spectra of the planetary nebula IC 418 were obtained in the wavelength range 4190-5850 A. The data made it possible to map an extended halo about the source, evaluate the variation in halo intensity with radius, and model the results in terms of a radially symmetric dust scatter envelope. It is suggested that the nebula is in a relatively
    Phillips, J. P. et al.

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    8
    1990
    Citations
    10
  • The Counterjet of HH 30: New Light on Its Binary Driving Source
    We present new [S II] images of the Herbig-Haro (HH) 30 jet and counterjet observed in 2006, 2007, and 2010 that, combined with previous data, allowed us to measure with improved accuracy the positions and proper motions of the jet and counterjet knots. Our results show that the motion of the knots is essentially ballistic, with the exception of
    Estalella, Robert et al.

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    8
    2012
    Citations
    28