activity
20022026
most citedThe Landscape of the Neutrino Mechanism of Core-Collapse Supernovae: Neutron Star and Black Hole Mass Functions, Explosion Energies and Nickel Yields

244 citations · 3.3k across the 56 of their papers we have counts for

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Showing astro-ph.HEShow all

11 papers · 1 filter

astro-ph.HE2026

Quantifying the impact of relativistic precession on tidal disruption event light curves

Diego Calderón, Ondřej Pejcha, Brian D. Metzger +2

The tidal field of a black hole can turn a star into a gas stream whose orbit can precess, especially if the a black hole is rapidly spinning. In this work, we investigate the impa…

astro-ph.HE2023★ 9 cited

The effect of relativistic precession on light curves of tidal disruption events

Diego Calderón, Ondřej Pejcha, Brian D. Metzger +1

The disruption of a star by the tidal forces of a spinning black hole causes the stellar stream to precess affecting the conditions for triggering the tidal disruption event (TDE).…

astro-ph.HE2023

Science with a small two-band UV-photometry mission I: Mission description and follow-up observations of stellar transients

N. Werner, J. Řípa, C. Thöne +33

This is the first in a collection of three papers introducing the science with an ultra-violet (UV) space telescope on an approximately 130~kg small satellite with a moderately fas…

astro-ph.HE2020

Direct evidence for shock-powered optical emission in a nova

Elias Aydi, Kirill V. Sokolovsky, Laura Chomiuk +39

Classical novae are thermonuclear explosions that occur on the surfaces of white dwarf stars in interacting binary systems (Bode & Evans 2008). It has long been thought that the lu…

astro-ph.HE2019★ 86 cited

The Type II-P Supernova 2017eaw: from explosion to the nebular phase

Tamás Szalai, József Vinkó, Réka Könyves-Tóth +36

The nearby SN 2017eaw is a Type II-P (``plateau') supernova showing early-time, moderate CSM interaction. We present a comprehensive study of this SN including the analysis of high…

astro-ph.HE2018★ 58 cited

A Comprehensive Analysis of Spitzer Supernovae

Tamás Szalai, Szanna Zsíros, Ori D. Fox +2

The mid-infrared (mid-IR) wavelength regime offers several advantages for following the late-time evolution of supernovae (SNe). First, the peaks of the SN spectral energy distribu…