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Primary and secondary source of energy in the superluminous supernova 2018ibb
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A Study of Primordial Very Massive Star Evolution
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Pulsational pair-instability supernovae in gravitational-wave and electromagnetic transients
D D Hendriks, L A C van Son, M Renzo, R G Izzard and R Farmer Monthly Notices of the Royal Astronomical Society 526(3) 4130 (2023) https://doi.org/10.1093/mnras/stad2857
Multidimensional Radiation Hydrodynamics Simulations of Pulsational Pair-instability Supernovae
Radio emission from a decade old Type I superluminous supernova, PTF10hgi: comparison with FRB121102
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Pulsation-driven Mass Loss from Massive Stars behind Stellar Mergers in Metal-poor Dense Clusters
Searches for Population III pair-instability supernovae: Predictions for ULTIMATE-Subaru and WFIRST
Takashi J Moriya, Kenneth C Wong, Yusei Koyama, Masaomi Tanaka, Masamune Oguri, Stefan Hilbert and Ken’ichi Nomoto Publications of the Astronomical Society of Japan 71(3) (2019) https://doi.org/10.1093/pasj/psz035
The Impact of Pair-instability Mass Loss on the Binary Black Hole Mass Distribution
Supernovae 2016bdu and 2005gl, and their link with SN 2009ip-like transients: another piece of the puzzle
A. Pastorello, C. S. Kochanek, M. Fraser, et al. Monthly Notices of the Royal Astronomical Society 474(1) 197 (2018) https://doi.org/10.1093/mnras/stx2668
Related Progenitor Models for Long-duration Gamma-Ray Bursts and Type Ic Superluminous Supernovae
David R. Aguilera-Dena, Norbert Langer, Takashi J. Moriya and Abel Schootemeijer The Astrophysical Journal 858(2) 115 (2018) https://doi.org/10.3847/1538-4357/aabfc1
Strange mode instabilities and mass loss in evolved massive primordial stars
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Stellar Yields of Rotating First Stars. II. Pair-instability Supernovae and Comparison with Observations
Variability of Red Supergiants in M31 from the Palomar Transient Factory
Monika D. Soraisam, Lars Bildsten, Maria R. Drout, Evan B. Bauer, Marat Gilfanov, Thomas Kupfer, Russ R. Laher, Frank Masci, Thomas A. Prince, Shrinivas R. Kulkarni, Thomas Matheson and Abhijit Saha The Astrophysical Journal 859(1) 73 (2018) https://doi.org/10.3847/1538-4357/aabc59
Red supergiant stars in the Large Magellanic Cloud
Immediate dense circumstellar environment of supernova progenitors caused by wind acceleration: its effect on supernova light curves
Takashi J. Moriya, Sung-Chul Yoon, Götz Gräfener and Sergei I. Blinnikov Monthly Notices of the Royal Astronomical Society: Letters 469(1) L108 (2017) https://doi.org/10.1093/mnrasl/slx056
Instability, finite amplitude pulsation and mass-loss in models of massive OB-type stars
Exact and approximate expressions of energy generation rates and their impact on the explosion properties of pair instability supernovae
Koh Takahashi, Takashi Yoshida, Hideyuki Umeda, Kohsuke Sumiyoshi and Shoichi Yamada Monthly Notices of the Royal Astronomical Society 456(2) 1320 (2016) https://doi.org/10.1093/mnras/stv2649
PTF13efv—AN OUTBURST 500 DAYS PRIOR TO THE SNHUNT 275 EXPLOSION AND ITS RADIATIVE EFFICIENCY
E. O. Ofek, S. B. Cenko, N. J. Shaviv, G. Duggan, N.-L. Strotjohann, A. Rubin, S. R. Kulkarni, A. Gal-Yam, M. Sullivan, Y. Cao, P. E. Nugent, M. M. Kasliwal, J. Sollerman, C. Fransson, A. V. Filippenko, D. A. Perley, O. Yaron and R. Laher The Astrophysical Journal 824(1) 6 (2016) https://doi.org/10.3847/0004-637X/824/1/6
How much radioactive nickel does ASASSN-15lh require?
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