T
Takashi J. Moriya
Researcher at National Institutes of Natural Sciences, Japan
Publications - 254
Citations - 7840
Takashi J. Moriya is an academic researcher from National Institutes of Natural Sciences, Japan. The author has contributed to research in topics: Supernova & Light curve. The author has an hindex of 43, co-authored 221 publications receiving 6495 citations. Previous affiliations of Takashi J. Moriya include University of Bonn & Monash University.
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Superluminous transients at AGN centers from interaction between black-hole disk winds and broad-line region clouds
TL;DR: In this article, superluminous transients that appear at central regions of active galactic nuclei (AGNs) such as CSS100217:102913+404220 (CSS100217) and PS16dtm, are powered by the interaction between accretion disk winds and clouds in broad-line regions (BLRs) surrounding them.
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Episodic modulations in supernova radio light curves from luminous blue variable supernova progenitor models
TL;DR: In this article, the authors investigated the link between LBV as SN progenitors and the appearance of episodic radio light curve modulations of the SN event and found that the 20Msun model shows radio light curves with episodic luminosity modulations, similar to those observed in some Type IIb SNe.
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The Quest for New Correlations in the Realm of the Gamma-Ray Burst—Supernova Connection
Maria Giovanna Dainotti,Biagi Simone,K. M. Islam,Kenji Kawaguchi,Takashi J. Moriya,Tomoya Takiwaki,Nozomu Tominaga,Anjasha Gangopadhyay +7 more
TL;DR: In this article , the authors investigated the existence of relationships among GRB prompt and afterglow (AG) properties and associated SN properties and found hints of a new correlation with a Pearson correlation coefficient > 0.50 and a probability of being drawn by chance < 0.05.
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Revealing the binary origin of Type Ic superluminous supernovae through nebular hydrogen emission
TL;DR: In this paper, a stripped mass of 0.1 -0.9 solar masses was derived for the Type Ia superluminous supernova iPTF13ehe.
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Euclid detectability of pair instability supernovae in binary population synthesis models consistent with merging binary black holes
TL;DR: In this article , the expected detection number of pair instability supernovae (PISNe) during the operation of the Euclid space telescope based on binary population models was derived.