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pro vyhledávání: '"Jeongmook Kim"'
Autor:
Gu Lim, Myungshin Im, Gregory S. H. Paek, Sung-Chul Yoon, Changsu Choi, Sophia Kim, J. Craig Wheeler, Benjamin P. Thomas, Jozsef Vinkó, Dohyeong Kim, Jinguk Seo, Wonseok Kang, Taewoo Kim, Hyun-Il Sung, Yonggi Kim, Joh-Na Yoon, Haeun Kim, Jeongmook Kim, Hana Bae, Shuhrat Ehgamberdiev, Otabek Burhonov, Davron Mirzaqulov
Publikováno v:
The Astrophysical Journal, Vol 949, Iss 1, p 33 (2023)
The progenitor system of Type Ia supernovae (SNe Ia) is expected to be a close binary system consisting of a carbon/oxygen white dwarf (WD) and a nondegenerate star or another WD. Here, we present results from high-cadence monitoring observations of
Externí odkaz:
https://doaj.org/article/05277b6147094df89715e582c5b44834
Autor:
Gu Lim, Myungshin Im, Gregory S. H. Paek, Sung-Chul Yoon, Changsu Choi, Sophia Kim, J. Craig Wheeler, Benjamin P. Thomas, Jozsef Vinkó, Dohyeong Kim, Jinguk Seo, Wonseok Kang, Taewoo Kim, Hyun-Il Sung, Yonggi Kim, Joh-Na Yoon, Haeun Kim, Jeongmook Kim, Hana Bae, Shuhrat Ehgamberdiev, Otabek Burhonov, Davron Mirzaqulov
The progenitor system of Type Ia supernovae (SNe Ia) is expected to be a close binary system of a carbon/oxygen white dwarf (WD) and a non-degenerate star or another WD. Here, we present results from a high-cadence monitoring observation of SN 2021hp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c01f5e8483c51e262e17482669d9508
