Astrophysical: Supernova remnants

  • Talk
    Observing the polarized microwave sky: 10 years of the QUIJOTE experiment
    I will review the status of the QUIJOTE (Q-U-I JOint TEnerife) experiment, a project led from the IAC with the aim of characterising the polarisation of the...
  • Talk
    3D-Imaging of the Molecular Emission from the Inner Debris of SN1987A (and the Dust Factory)
    Supernova SN1987A in the Large Magellanic Cloud offers an unprecedented opportunity to tackle fundamental issues of supernova explosions: dust and molecule...
  • Talk
    A message from Crab pulsar in Teraelectronvolt fonts
    Using ~320h of good-quality Crab data from Feb 2007 to Apr 2014 the MAGIC telescopes measured the most energetic pulsed photons from a pulsar to date. The new...
  • Publication
    A remarkable feature in the giant extragalactic H II region NGC 5471
    The discovery of a very high velocity, low-intensity gas feature in the giant extragalactic H II region NGC 5471 is reported. A broad component in the emission...
  • Publication
    An Integral View of Balmer-dominated Shocks in Supernova Remnants
    We present integral-field spectroscopic observations with the VIMOS-IFU at the VLT of fast (2000-3000 kms-1) Balmer-dominated shocks surrounding the...
  • Publication
    Balmer Filaments in Tycho’s Supernova Remnant: An Interplay between Cosmic-ray and Broad-neutral Precursors
    We present Hα spectroscopic observations and detailed modeling of the Balmer filaments in the supernova remnant (SNR) Tycho (SN 1572). We used GH α FaS (Galaxy...
  • Publication
    Cosmic-ray acceleration and escape from supernova remnant W44 as probed by Fermi-LAT and MAGIC
    Context. The supernova remnant (SNR) W44 and its surroundings are a prime target for studying the acceleration of cosmic rays (CRs). Several previous studies...
  • Publication
    Detailed study of the microwave emission of the supernova remnant 3C 396
    We have observed the supernova remnant 3C 396 in the microwave region using the Parkes 64-m telescope. Observations have been made at 8.4, 13.5, and 18.6 GHz...
  • Publication
    Detection and measurement of expanding ionized shells around young star clusters
    We present a new method (BUBBLY) for detecting expanding components of ionized gas using integral field spectroscopy, showing its capabilities not only in...