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20212026
most citedPrecursors of Supernovae from Mass Eruption: Prospects for Early Warning of Nearby Core-collapse Supernovae

22 citations · 91 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

Probing the Nature of the Circumstellar Material Surrounding SN 2024ggi: A Search for Precursor Emission and Constraints from Radio Observations

Tobias Géron, James K. Leung, Maria R. Drout +8

We present an analysis of the pre-explosion optical light curve and post-explosion radio observations of the nearby supernova (SN) 2024ggi, a Type II SN discovered in NGC 3621 at a…

astro-ph.SR2025★ 4 cited

Population Synthesis Study on the Binary Origin of Type Ibn Supernovae

Takatoshi Ko, Tomoya Kinugawa, Daichi Tsuna +2

Type Ibn supernovae (SNe) are a class of SN explosions whose progenitors are surrounded by dense helium-rich circumstellar matter (CSM). Some models have been proposed for how to f…

astro-ph.SR2025

Confined Circumstellar Material as a Dust Formation Site in Type II Supernovae

Yuki Takei, Kunihito Ioka, Masaru Shibata

We propose a model for dust formation in Type II supernovae (SNe) interacting with confined circumstellar material (CSM), motivated by recent time-domain surveys that have revealed…

astro-ph.HE2024★ 17 cited

A cosmic formation site of silicon and sulphur revealed by a new type of supernova explosion

Steve Schulze, Avishay Gal-Yam, Luc Dessart +47

The cores of stars are the cosmic furnaces where light elements are fused into heavier nuclei. The fusion of hydrogen to helium initially powers all stars. The ashes of the fusion…

astro-ph.HE2024★ 1 cited

Detached Circumstellar Matter as an Explanation for Slowly-Rising Interacting Type Ibc Supernovae

Yuki Takei, Daichi Tsuna

Some hydrogen-poor (Type Ibc) supernovae (SNe) are known to have massive circumstellar matter (CSM) that are well detached from the star. Using the open-source code CHIPS, we const…

astro-ph.HE2023

Diagnosis of Circumstellar Matter Structure in Interaction-powered Supernovae with Hydrogen Line Feature

Ayako T. Ishii, Yuki Takei, Daichi Tsuna +2

Some supernovae (SNe) are powered by collision of the SN ejecta with a dense circumstellar matter (CSM). Their emission spectra show characteristic line shapes of combined broad em…

astro-ph.HE2023

Simulating Hydrogen-poor Interaction-Powered Supernovae with CHIPS

Yuki Takei, Daichi Tsuna, Takatoshi Ko +1

We present the updated open-source code Complete History of Interaction-Powered Supernovae (CHIPS) that can be applied to modeling supernovae (SNe) arising from an interaction with…

astro-ph.HE2023★ 12 cited

Detached and Continuous Circumstellar Matter in Type Ibc Supernovae from Mass Eruption

Daichi Tsuna, Yuki Takei

Some hydrogen-poor supernovae (SNe) are found to undergo interaction with dense circumstellar matter (CSM) that may originate from mass eruption(s) just prior to core-collapse. We…

astro-ph.HE2022★ 22 cited

Precursors of Supernovae from Mass Eruption: Prospects for Early Warning of Nearby Core-collapse Supernovae

Daichi Tsuna, Yuki Takei, Toshikazu Shigeyama

Recent observations of a large fraction of Type II supernovae show traces of dense circumstellar medium (CSM) very close to the progenitor star. If this CSM is created by eruptive…

astro-ph.SR2021★ 18 cited

Eruption of the Envelope of Massive Stars by Energy Injection with Finite Duration

Takatoshi Ko, Daichi Tsuna, Yuki Takei +1

A significant fraction of supernovae show signatures of dense circumstellar material (CSM). While multiple scenarios for creating a dense CSM exist, mass eruption due to injection…

astro-ph.HE2021★ 17 cited

CHIPS: Complete History of Interaction-Powered Supernovae

Yuki Takei, Daichi Tsuna, Naoto Kuriyama +2

We present the public release of the Complete History of Interaction-Powered Supernovae (CHIPS) code, suited to model a variety of transients that arise from interaction with a den…