:https://www.wis-tns.org/object/2023yoa
CBAT页面链接:http://www.cbat.eps.harvard.edu/unconf/followups/J00430932 ...
:https://www.wis-tns.org/object/2023ypg
CBAT页面链接:http://www.cbat.eps.harvard.edu/unconf/followups/J01325400 ...
:https://www.wis-tns.org/object/2023yqt
CBAT页面链接:http://www.cbat.eps.harvard.edu/unconf/followups/J00422755 ...
:https://www.wis-tns.org/object/2023yvj
CBAT页面链接:http://www.cbat.eps.harvard.edu/unconf/followups/J00452890 ...
该新星系统包含1颗大于1.36倍太阳质量的白矮星,白矮星通过吸积伴星物质的方式增加质量;同时,这颗白矮星发生新星爆炸抛射的物质质量比吸积的物质质量要小,因此它可能会在数十万年内爆炸为Ia型超新星或坍缩为中子星 ...