Abstract
In this work, we study the synthetic explosions of a massive star. We take a 100 \(M_{\odot }\) zero-age main-sequence (ZAMS) star and evolve it until the onset of core-collapse using MESA. Then, the resulting star model is exploded using the publicly available stellar explosion code, STELLA. The outputs of STELLA calculations provide the bolometric light curve and photospheric velocity evolution along with other physical properties of the underlying supernova. In this paper, the effects of having a large Hydrogen-envelope on the supernova light curve have been explored. We also explore the effects of the presence of different amounts of nickel mass and the variation of the explosion energy of the supernovae from such heavy progenitors, on the bolometric light curves and photospheric velocities.
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Acknowledgments
The authors would like to thank the anonymous referee for providing valuable comments. Amar Aryan acknowledges funds and assistance provided by the Council of Scientific & Industrial Research (CSIR), India with file no. 09/948(0003)/2020-EMR-I. A.A., S.B.P. and R.G. acknowledge BRICS grant DST/IMRCD/BRICS/Pilotcall/ProFCheap/2017(G). The authors are also thankful to the MESA troubleshooting team for their constant support and guidance.
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This article is part of the Special Issue on "Astrophysical Jets and Observational Facilities: A National Perspective".
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ARYAN, A., PANDEY, S.B., YADAV, A.P. et al. Core-collapse supernova from a possible progenitor star of 100 \(M_{\odot }\). J Astrophys Astron 43, 2 (2022). https://doi.org/10.1007/s12036-021-09784-6
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DOI: https://doi.org/10.1007/s12036-021-09784-6