activity
20112020
most citedSelf-consistent 3D Supernova Models From -7 Minutes to +7 Seconds: a 1-bethe Explosion of a ~19 Solar-mass Progenitor

187 citations · 506 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2020★ 187 cited

Self-consistent 3D Supernova Models From -7 Minutes to +7 Seconds: a 1-bethe Explosion of a ~19 Solar-mass Progenitor

R. Bollig, N. Yadav, D. Kresse +3

To date, modern three-dimensional (3D) supernova (SN) simulations have not demonstrated that explosion energies of 10^{51} erg (=1 bethe = 1B) or more are possible for neutrino-dri…

astro-ph.HE2019★ 82 cited

Large-Scale Mixing in a Violent Oxygen-Neon Shell Merger Prior to a Core-Collapse Supernova

Naveen Yadav, Bernhard Müller, Hans Thomas Janka +2

We present a seven-minute long -3D simulation of a shell merger event in a non-rotating supernova progenitor before the onset of gravitational collapse. The k…

astro-ph.HE2016★ 7 cited

Low frequency radio observations of SN 2011dh and the evolution of its post-shock plasma properties

Naveen Yadav, Alak Ray, Sayan Chakraborti

We present late time, low frequency observations of SN 2011dh made using the Giant Metrewave Radio Telescope (GMRT). Our observations at , and $1280\ \…

astro-ph.HE2016★ 77 cited

How multiple supernovae overlap to form superbubbles

Naveen Yadav, Dipanjan Mukherjee, Prateek Sharma +1

We explore the formation of superbubbles through energy deposition by multiple supernovae (SNe) in a uniform medium. We use total energy conserving, 3-D hydrodynamic simulations to…

astro-ph.HE2014★ 53 cited

A Missing-Link in the Supernova-GRB Connection: The Case of SN 2012ap

Sayan Chakraborti, Alicia Soderberg, Laura Chomiuk +50

Gamma Ray Bursts (GRBs) are characterized by ultra-relativistic outflows, while supernovae are generally characterized by non-relativistic ejecta. GRB afterglows decelerate rapidly…

astro-ph.HE2013★ 24 cited

Electron Cooling in a Young Radio Supernova: SN 2012aw

Naveen Yadav, Alak Ray, Sayan Chakraborti +8

We present the radio observations and modeling of an optically bright Type II-P supernova (SN), SN 2012aw which exploded in the nearby galaxy Messier 95 (M95) at a distance of $10\…

astro-ph.HE2013★ 29 cited

The progenitor of SN 2011ja: Clues from circumstellar interaction

Sayan Chakraborti, Alak Ray, Randall Smith +7

Massive stars, possibly red supergiants, which retain extended hydrogen envelopes until core collapse, produce Type II Plateau (IIP) supernovae. The ejecta from these explosions sh…

astro-ph.HE2012★ 23 cited

X-Ray emission from SN 2004dj: A Tale of Two Shocks

Sayan Chakraborti, Naveen Yadav, Alak Ray +2

Type IIP (Plateau) Supernovae are the most commonly observed variety of core collapse events. They have been detected in a wide range of wavelengths from radio, through optical to…

astro-ph.CO2011★ 24 cited

Radio Detection of Green Peas: Implications for Magnetic Fields in Young Galaxies

Sayan Chakraborti, Naveen Yadav, Carolin Cardamone +1

Green Peas are a new class of young, emission line galaxies that were discovered by citizen volunteers in the Galaxy Zoo project. Their low stellar mass, low metallicity and very h…