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20112025
most citedConfined Dense Circumstellar Material Surrounding a Regular Type II Supernova: The Unique Flash-Spectroscopy Event of SN 2013fs

377 citations · 740 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2025★ 4 cited

The Optical to X-ray Luminosity and Spectrum of Supernova Wind Breakouts

Tal Wasserman, Nir Sapir, Peter Szabo +1

Observations indicate that optically thick circum-stellar medium (CSM) at radii of cm around Type II core-collapse supernovae (SN) progenitors is common (and may…

astro-ph.HE2024

Shock cooling emission from explosions of massive stars: III. Blue Super Giants

J. Morag, N. Sapir, E. Waxman

Light emission in the first hours and days following core-collapse supernovae is dominated by the escape of photons from the expanding shock-heated envelope. In preceding papers, w…

astro-ph.HE2023

Shock cooling emission from explosions of red super-giants: II. An analytic model of deviations from blackbody emission

Jonathan Morag, Ido Irani, Nir Sapir +1

Light emission in the first hours and days following core-collapse supernovae (SNe) is dominated by the escape of photons from the expanding shock heated envelope. In a preceding p…

astro-ph.HE2022★ 39 cited

Shock cooling emission from explosions of red super-giants: I. A numerically calibrated analytic model

Jonathan Morag, Nir Sapir, Eli Waxman

Supernova light curves are dominated at early time, hours to days, by the escape of photons from the expanding shock heated envelope. We provide a simple analytic description of th…

astro-ph.HE2017★ 377 cited

Confined Dense Circumstellar Material Surrounding a Regular Type II Supernova: The Unique Flash-Spectroscopy Event of SN 2013fs

O. Yaron, D. A. Perley, A. Gal-Yam +30

With the advent of new wide-field, high-cadence optical transient surveys, our understanding of the diversity of core-collapse supernovae has grown tremendously in the last decade.…

astro-ph.HE2016★ 94 cited

UV/Optical emission from the expanding envelopes of type II supernovae

Nir Sapir, Eli Waxman

The early part of a supernova (SN) light-curve is dominated by radiation escaping from the expanding shock-heated progenitor envelope. For polytropic Hydrogen envelopes, the proper…