We present partial results from our monitoring of the nuclear region of the starburst galaxy IC 694 (=Arp 299-A) at radio wavelengths, aimed at discovering recently exploded core-collapse supernovae, as well as to determine their rate of explosion, which carries crucial information on star formation rates and starburst scenarios at work. Two epochs of eEVN observations at 5.0 GHz, taken in 2008, revealed the presence of a rich cluster of compact radio emitting sources in the central 150 pc of the nuclear starburst in Arp 299A. The large brightness temperatures observed for the compact sources indicate a non-thermal origin for the observed radio emission, implying that most, if not all, of those sources were young radio supernovae and supern...
Only a few cases of Type Ic supernovae (SNe) with high-velocity ejecta (≥0.2 c) have been discovered...
SUPERNOVA explosions are poorly understood, partly because of difficulties in modelling them theoret...
We present results from 4.8 GHz Very Large Array (VLA) and global very long baseline interferometry ...
Context. The central kiloparsec of many local uminous infrared galaxies are known to host intense bu...
Context. The dusty nuclear regions of luminous infra-red galaxies (LIRGs) are heated by either an i...
We report radio observations of two stripped-envelope supernovae (SNe), 2010O and 2010P, which explo...
We report on 1.6- and 5.0-GHz observations of the ultraluminous infrared galaxy (ULIRG) Mrk 273, usi...
We report on 1.6 and 5.0 GHz observations of the ultraluminous infrared galaxy (ULIRG) Mrk 273, usin...
Using a long (150 ks) broadband (0.1-40 keV) BeppoSAX observation of the merging starburst system Ar...
In this Letter, we report the discovery of a new bright radio transient in M 82. Using the Very Lar...
Context. The two nuclei of the starburst galaxy Arp220 contain multiple compact radio sources previo...
Data accumulated over the past year strongly favour the idea that γ-ray bursts lie at cosmological d...
We report the first detection at multiple radio wavelengths (13, 6, and 3.6 cm) of 18 compact source...
We present mid-infrared (MIR) 8-13 μm spectroscopy of the nuclear regions of the interacting galaxy ...
We present results from 4.8 GHz Very Large Array (VLA) and global very long baseline interferometry ...
Only a few cases of Type Ic supernovae (SNe) with high-velocity ejecta (≥0.2 c) have been discovered...
SUPERNOVA explosions are poorly understood, partly because of difficulties in modelling them theoret...
We present results from 4.8 GHz Very Large Array (VLA) and global very long baseline interferometry ...
Context. The central kiloparsec of many local uminous infrared galaxies are known to host intense bu...
Context. The dusty nuclear regions of luminous infra-red galaxies (LIRGs) are heated by either an i...
We report radio observations of two stripped-envelope supernovae (SNe), 2010O and 2010P, which explo...
We report on 1.6- and 5.0-GHz observations of the ultraluminous infrared galaxy (ULIRG) Mrk 273, usi...
We report on 1.6 and 5.0 GHz observations of the ultraluminous infrared galaxy (ULIRG) Mrk 273, usin...
Using a long (150 ks) broadband (0.1-40 keV) BeppoSAX observation of the merging starburst system Ar...
In this Letter, we report the discovery of a new bright radio transient in M 82. Using the Very Lar...
Context. The two nuclei of the starburst galaxy Arp220 contain multiple compact radio sources previo...
Data accumulated over the past year strongly favour the idea that γ-ray bursts lie at cosmological d...
We report the first detection at multiple radio wavelengths (13, 6, and 3.6 cm) of 18 compact source...
We present mid-infrared (MIR) 8-13 μm spectroscopy of the nuclear regions of the interacting galaxy ...
We present results from 4.8 GHz Very Large Array (VLA) and global very long baseline interferometry ...
Only a few cases of Type Ic supernovae (SNe) with high-velocity ejecta (≥0.2 c) have been discovered...
SUPERNOVA explosions are poorly understood, partly because of difficulties in modelling them theoret...
We present results from 4.8 GHz Very Large Array (VLA) and global very long baseline interferometry ...