A low-mass helium star progenitor model for the Type Ibn SN 2020nxt
Qinan Wang, Anika Goel, Luc Dessart, Ori D. Fox, Melissa Shahbandeh, S. Rest, A. Rest, J. H. Groh, Andrew Allan, Claes Fransson, Nathan Smith, G. Hosseinzadeh, Alexei V Filippenko, Jennifer E. Andrews, K. Azalee Bostroem, Thomas G. Brink, P. J. Brown, J. Burke, Roger A. Chevalier, Geoffrey C. Clayton, Mi Dai, Kyle W. Davis, R. J. Foley, Sebastián Gómez, Chelsea Harris, D. Hiramatsu, D. A. Howell, Connor Jennings, Saurabh W. Jha, M. M. Kasliwal, Patrick L. Kelly, Erik C. Kool, Evelyn Liu, Emily Ma, C. McCully, Adam A. Miller, Yukei S. Murakami, Estefania Padilla Gonzalez, C. Pellegrino, Derek Perera, Justin Pierel, C. Rojas-Bravo, M. R. Siebert, J. Sollerman, Tamás Szalai, Samaporn Tinyanont, Schuyler D. Van Dyk, WeiKang Zheng, K. C. Chambers, D. A. Coulter, Thomas de Boer, N. Earl, D. Farias, C. Gall, Peter McGill, C. L. Ransome, K. Taggart, V. Ashley Villar (2024). A low-mass helium star progenitor model for the Type Ibn SN 2020nxt. , 530(4), DOI: https://doi.org/10.1093/mnras/stae1038.
