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/

  • Energy in density gradient
    Inhomogeneous plasmas and fluids contain energy stored in inhomogeneity and they naturally tend to relax into lower energy states by developing instabilities or by diffusion. But the actual amount of energy in such inhomogeneities has remained unknown. In the present work, the amount of energy stored in a density gradient is calculated for several
    Vranjes, J. et al.

    Advertised on:

    1
    2015
    Citations
    0
  • Dissecting galactic bulges in space and time - I. The importance of early formation scenarios versus secular evolution
    The details of bulge formation via collapse, mergers, secular processes or their interplay remain unresolved. To start answering this question and quantify the importance of distinct mechanisms, we mapped a sample of three galactic bulges using data from the integral field spectrograph WiFeS on the ANU's 2.3-m telescope in Siding Spring Observatory
    Seidel, M. K. et al.

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    1
    2015
    Citations
    31
  • Discovery of very high energy γ-ray emission from the blazar 1ES 0033+595 by the MAGIC telescopes
    The number of known very high energy (VHE) blazars is ˜50, which is very small in comparison to the number of blazars detected in other frequencies. This situation is a handicap for population studies of blazars, which emit about half of their luminosity in the γ-ray domain. Moreover, VHE blazars, if distant, allow for the study of the environment
    Aleksić, J. et al.

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    1
    2015
    Citations
    16
  • Differences between CO- and calcium triplet-derived velocity dispersions in spiral galaxies: evidence for central star formation?
    We examine the stellar velocity dispersions (σ) of a sample of 48 galaxies, 35 of which are spirals, from the Palomar nearby galaxy survey. It is known that for ultra-luminous infrared galaxies (ULIRGs) and merger remnants, the σ derived from the near-infrared CO band heads is smaller than that measured from optical lines, while no discrepancy
    Riffel, R. A. et al.

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    1
    2015
    Citations
    20
  • Detection of Neodymium in APOGEE H-band Spectra and its Application to Chemical Tagging
    We report the successful detection of the rare earth element Neodymium (Nd) in the high-resolution, H-band spectra from the SDSS III Apache Point Observatory Galactic Evolution Experiment (APOGEE). Using the Nd II transition at 16058.014 angstroms, we have detected significant Nd enhancements in all stars observed by APOGEE belonging to the
    Hasselquist, S. et al.

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    1
    2015
    Citations
    0
  • Detailed Magnetic Field Morphology of the Vela C Molecular Cloud from the BLASTPol 2012 flight
    In order to understand the role of magnetic fields in the process of star formation, we require detailed observations of field morphology on scales ranging from clouds to cores. However, ground based millimetre/submillimetre polarimetry is usually limited to small maps of relatively dense regions. BLASTPol, the Balloon-borne Large Aperture Sub-mm
    Fissel, L. M. et al.

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    1
    2015
    Citations
    0