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机译:来自K2的证据在中间质子星的后代迅速旋转
Univ N Carolina Dept Phys &
Astron Chapel Hill NC 27599 USA;
Iowa State Univ Dept Phys &
Astron Ames IA 50011 USA;
Univ Fed Rio Grande do Sul Inst Fis Porto Alegre RS Brazil;
Univ Fed Rio Grande do Sul Inst Fis Porto Alegre RS Brazil;
Univ Warwick Dept Phys Coventry CV4 7AL W Midlands England;
Univ Texas Austin Dept Astron Austin TX 78712 USA;
Univ N Carolina Dept Phys &
Astron Chapel Hill NC 27599 USA;
Univ Texas Austin Dept Astron Austin TX 78712 USA;
Univ Warwick Dept Phys Coventry CV4 7AL W Midlands England;
Univ N Carolina Dept Phys &
Astron Chapel Hill NC 27599 USA;
Univ N Carolina Dept Phys &
Astron Chapel Hill NC 27599 USA;
Wesleyan Univ Astron Dept Van Vleck Observ 96 Foss Hill Dr Middletown CT 06459 USA;
stars: individual (EPIC 211914185); stars: oscillations (including pulsations); stars: rotation; white dwarfs;
机译:来自K2的证据在中间质子星的后代迅速旋转
机译:快速旋转的恒星的脉动-II。中等质量恒星的逼真建模
机译:重力惯性模式对中等质量主序星旋转差的敏感性
机译:X射线双星及其后代:二进制无线电脉冲;证明三类中子星?
机译:详细的外边界条件对中质星演化的影响
机译:年轻的原恒星Barnard 1b-N和S中的化学偏析Barnard 1b-S中伪盘旋转的证据
机译:来自K2的证据,证实了一颗中等质量恒星的后代快速旋转