SN 2022oqm：来自白矮星双星前体系统的多峰钙丰富暂现
摘要：SN 2022oqm的光度和光谱演化：一种邻近的多峰氢和氦弱的富含钙的短暂现象。
作者：S. Karthik Yadavalli, V. Ashley Villar, Luca Izzo, Yossef Zenati, Ryan J. Foley, J. Craig Wheeler, Charlotte R. Angus, Dominik B''anhidi, Katie Auchettl, Barna Imre B''ir''o, Attila B''odi, Zs''ofia Bodola, Thomas de Boer, Kenneth C. Chambers, Ryan Chornock, David A. Coulter, Istv''an Cs''anyi, Borb''ala Cseh, Srujan Dandu, Kyle W. Davis, Connor Braden Dickinson, Diego Farias, Christa Gall, Hua Gao, Wynn V. Jacobson-Galan, Nandita Khetan, Charles D. Kilpatrick, R''eka K"onyves-T''oth, Levente Kriskovics, Natalie LeBaron, Kayla Loertscher, X. K. Le Saux, Rafaella Margutti, Eugene A. Magnier, Peter McGill, Hao-Yu Miao, Andr''as P''al, Bor''oka H. P''al, Yen-Chen Pan, Collin A. Politsch, Conor L. Ransome, Enrico Ramirez-Ruiz, Armin Rest, Sofia Rest, Olivia Robinson, Huei Sears, Jackson Scheer, ''Ad''am S''odor, Jonathan Swift, P''eter Sz''ekely, R''obert Szak''ats, Tam''as Szalai, Kirsty Taggart, Padma Venkatraman, J''ozsef Vink''o, Grace Yang, Henry Zhou
论文ID：2308.12991
分类：High Energy Astrophysical Phenomena
分类简称：astro-ph.HE
提交时间：2023-08-31