activity
20172021
most citedMagnetar-Powered Supernovae in Two Dimensions. II. Broad-Line Supernovae Ic

28 citations · 47 across the 5 of their papers we have counts for

collaborators

9 papers

nucl-ex20217 cited

Progress in Nuclear Astrophysics of East and Southeast Asia

Azni Abdul Aziz, Nor Sofiah Ahmad, S. Ahn +25

Nuclear astrophysics is an interdisciplinary research field of nuclear physics and astrophysics, seeking for the answer to a question, how to understand the evolution of the Univer…

astro-ph.HE202111 cited

Physics of Superluminous Supernovae

Ke-Jung Chen

Understanding how massive stars die as supernovae is a crucial question in modern astrophysics. Supernovae are powerful stellar explosions and key drivers in the cosmic baryonic cy…

astro-ph.HE2021

Observational properties of a general relativistic instability supernova from a primordial supermassive star

Takashi J. Moriya, Ke-Jung Chen, Kimihiko Nakajima +2

We present the expected observational properties of a general relativistic instability supernova (GRSN) from the 55,500 Msun primordial (Population III) star. Supermassive stars ex…

astro-ph.GA20201 cited

How the Population III Initial Mass Function Governs the Properties of the First Galaxies

Li-Hsin Chen, Ke-Jung Chen, Sung-han Tsai +1

The properties of Population III (Pop III) stars impact many aspects of primeval structure formation such as the onset of cosmological reionization and early chemical enrichment. H…

astro-ph.HE2019

Gas Dynamics of the Nickel-56 Decay Heating in Pair-Instability Supernovae

Ke-Jung Chen, S. E. Woosley, Daniel J. Whalen

Very massive 140-260 Msun stars can die as highly-energetic pair-instability supernovae (PI SNe) with energies of up to 100 times those of core-collapse SNe that can completely des…

astro-ph.HE2019

Three-Dimensional Simulations of Magnetar-Powered Superluminous Supernovae

Ke-Jung Chen, S. E. Woosley, Daniel J. Whalen

A rapidly spinning magnetar in a young supernova (SN) can produce a superluminous transient by converting a fraction of its rotational energy into radiation. Here, we present the f…