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
    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...

  • Publication
    Discovery of TeV γ-ray emission from the neighbourhood of the supernova remnant G24.7+0.6 by MAGIC

    SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV regime, SNR G24.7+0.6 (3FHL J1834.1-0706e/FGES J1834.1-0706...