机译:超软X射线源的数量:新星,潮汐破坏,Ia型超新星,吸积引起的坍塌,电离和中等质量的黑洞?
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138;
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138;
Institute of Astronomy and Department of Physics, National Tsing Hua University, Hsinchu 30013, Taiwan;
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138|Department of Physics and Astronomy, Rutgers University;
black hole physics; galaxies: general; nova, cataclysmic variables; stars: neutron; supernovae: general; white dwarfs; X-rays: binaries; X-rays: ISM;
机译:超软X射线源的数量:新星,潮汐破坏,Ia型超新星,吸积引起的坍塌,电离和中等质量的黑洞?
机译:超软X射线源和Ia型超新星的祖先
机译:超软X射线源和Ia型超新星的祖先
机译:IA型Supernovae和Supersoft X射线源
机译:吸积磁盘不稳定性的主题:I.中间极的磁化磁盘和GK Per,以及II。黑洞X射线新星中的辐照圆盘
机译:吸积引起的变异性将年轻的恒星物体白矮星和黑洞联系起来
机译:supersoft X射线源的种群:Novae,潮汐破坏,Ia型超新星,吸积诱导坍塌,电离和中等质量黑洞?
机译:发光的超软X射线源作为Ia型超新星的祖先