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Late-time radio and millimeter observations of superluminous supernovae and long gamma-ray bursts: Implications for central engines, fast radio bursts, and obscured star formation

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This article is published in The Astrophysical Journal.The article was published on 2021-05-01 and is currently open access. It has received 16 citations till now. The article focuses on the topics: Gamma-ray burst & Stellar physics.

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Gamma-Ray Thermalization and Leakage from Millisecond Magnetar Nebulae: Toward a Self-consistent Model for Superluminous Supernovae

TL;DR: In this article, the authors track the evolution of photons and matter in a coupled two-zone ("wind/nebula" and "ejecta") model, accounting for the range of radiative processes, and identify a mechanism by which gamma-gamma pair creation in the upstream pulsar wind regulates the mean energy of particles entering the nebula over the first several years after the explosion.
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Superluminous supernovae: an explosive decade

TL;DR: In this article, the authors review the current understanding of superluminous supernovae, mysterious events 100 times brighter than conventional stellar explosions, and present a review of the state of the art.
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The Zwicky Transient Facility phase I sample of hydrogen-rich superluminous supernovae without strong narrow emission lines

TL;DR: In this paper , the authors examined the light curves and spectra of 14 hydrogen-rich superluminous supernovae (SLSNeII) from the Zwicky Transient Facility (ZTF) between 2018 and 2020 and attempted to constrain their power source using light-curve models.
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Post maximum light and late time optical imaging polarimetry of type I superluminous supernova 2020znr

TL;DR: In this paper , optical imaging polarimetry was conducted on the hydrogen poor superluminous supernova 2020znr during 3 phases after maximum light (≈ +34 days, +288 days and +289 days).
Journal ArticleDOI

On the diversity of magnetar-driven kilonovae

TL;DR: In this article , the role of the magnetic field strength of binary neutron star mergers and the resulting electromagnetic signatures as a function of the external dipolar and internal toroidal fields was studied.
References
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Collapsars: Gamma-ray bursts and explosions in 'failed supernovae'

TL;DR: In this paper, the authors explore the continued evolution of rotating helium stars, Mα 10 M☉, in which iron-core collapse does not produce a successful outgoing shock but instead forms a black hole of 2-3 Mˉ.
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Planck 2015 results. I. Overview of products and scientific results

R. Adam, +353 more
TL;DR: The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14~May 2009 and scanned the microwave and submillimetre sky continuously between 12~August 2009 and 23~October 2013 as discussed by the authors.
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Jets in Gamma-Ray Bursts

TL;DR: In the afterglows of several gamma-ray bursts (GRBs), rapid temporal decay, which is inconsistent with spherical (isotropic) blastwave models, is observed as mentioned in this paper.
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