30 citations · 70 across the 7 of their papers we have counts for
5 papers · 1 filter
The Most Luminous Known Fast Blue Optical Transient AT 2024wpp: Unprecedented Evolution and Properties in the X-rays and Radio
A. J. Nayana, Raffaella Margutti, Eli Wiston +34
We present X-ray (0.3--79 keV) and radio (0.25--203 GHz) observations of the most luminous Fast Blue Optical Transient (LFBOT) AT\,2024wpp at , spanning 2--280 days after…
Dinosaur in a Haystack : X-ray View of the Entrails of SN 2023ixf and the Radio Afterglow of Its Interaction with the Medium Spawned by the Progenitor Star (Paper 1)
A. J. Nayana, Raffaella Margutti, Eli Wiston +24
We present the results from our extensive hard-to-soft X-ray (NuSTAR, Swift-XRT, XMM-Newton, Chandra) and meter-to-mm wave radio (GMRT, VLA, NOEMA) monitoring campaign of the very…
Hypercritical accretion during common envelopes in triples leading to binary black holes in the pair-instability-supernova mass gap
Enrique Moreno Méndez, Fabio De Colle, Diego López Cámara +1
Hydrodynamic studies of stellar-mass compact objects (COs) in a common envelope (CE)have shown that the accretion rate onto the CO is a few orders of magnitude below the Bondi-Hoyl…
Radio emission from the cocoon of a GRB jet: implications for relativistic supernovae and off-axis GRB emission
Fabio De Colle, Pawan Kumar, David R. Aguilera-Dena
Relativistic supernovae constitute a sub-class of type Ic supernovae (SNe). Their non-thermal, radio emission differs notably from that of regular type Ic supernovae as they have a…
Origin of the bilateral structure of the supernova remnant G296.5+10
A. Moranchel-Basurto, P. F. Velázquez, E. Giacani +4
In the present work we have modeled the supernova remnant (SNR) G296.5+10, by means of 3D magnetohydrodynamics (MHD) simulations. This remnant belongs to the bilateral SNR group an…