An Integral View of Fast Shocks around Supernova 1006.
Supernova remnants are among the most spectacular examples of astrophysical pistons in our cosmic neighborhood. The gas expelled by the supernova explosion is...
An Interacting Binary System Powers Precessing Outflows of an Evolved Star.
Stars are generally spherical, yet their gaseous envelopes oftenappear non-spherical when ejected near the end of their lives. Thisquirk is most notable during...
An ionised bubble powered by a proto-cluster at z = 6.5
We show herein that a proto-cluster of Lyα emitting galaxies, spectroscopically confirmed at redshift 6.5, produces a remarkable number of ionising continuum...
An ultraviolet wind in a neutron star X-ray binary transient
All disc-accreting astrophysical objects produce powerful disc winds. In compact binaries containing neutron stars or black holes, accretion often takes place...
Anomalous microwave emission detected from the Taurus Molecular Cloud with the QUIJOTE experiment
The QUIJOTE experiment operates from the Teide Observatory with the goal of characterising the polarization properties of the cosmic microwave background...
Appraising the Necklace: A post-common-envelope carbon dwarf inside an apparently carbon-poor planetary nebula
The Necklace nebula is a bipolar, post-common-envelope planetary nebula, the central star of which has been shown to have a dwarf carbon star companion. We aim...
Después de las campañas realizadas en los últimos cuatro años, la reducción y análisis de la mayoría de los datos y la publicación de los mismos (Shaltout y...
Are solar chromospheric fibrils tracing the magnetic field?
Fibrils are thin elongated features visible in the solar chromosphere in and around magnetized regions. Because of their visual appearance they have been...
Are Tornado-Like Magnetic Structures Able To Support Solar Prominence Plasma?
Recent high-resolution and high-cadence observations have surprisingly suggested that prominence barbs exhibit apparent rotating motions suggestive of a tornado...