机译:球状星团M 30中两个蓝色散乱星的不同序列
Department of Astronomy, University of Bologna, Via Ranzani 1, 40127 Bologna, Italy;
ESA, Space Science Department, Keplerlaan 1, 2200 AG Noordwijk, Netherlands;
Department of Astronomy, University of Bologna, Via Ranzani 1, 40127 Bologna, Italy;
Department of Astronomy, University of Bologna, Via Ranzani 1, 40127 Bologna, Italy;
McMaster University, Department of Physics and Astronomy, 1280 Main Street West, Hamilton, Ontario L8S 4M1, Canada.;
Astronomy Department, University of Virginia, PO Box 400325,Charlottesville, Virginia 22904, USA;
INAF, Osservatorio Astronomico di Bologna, Via Ranzani 1,40127 Bologna, Italy;
Research School of Astronomy and Astrophysics, Mt Stromlo Observatory, Weston Creek, Australian Capital Territory 2611, Australia;
Department of Astronomy, University of Bologna, Via Ranzani 1, 40127 Bologna, Italy;
Department of Astronomy, University of Bologna, Via Ranzani 1, 40127 Bologna, Italy;
机译:球形团簇中的蓝色散漫星族。 I.蓝色散子星在NGC?3201,NGC?6218和ωCENTAURI中的动力学特性
机译:球状星团中主序星的碰撞和蓝色条纹的形成
机译:球状星团中主序星的碰撞和蓝色条纹的形成
机译:在银河球簇中的蓝色孤立颗星:追踪动力学对恒星演化的影响
机译:旧的开放星团NGC 188中的双星和蓝色散落者
机译:球状星团与高速恒星之间的可能关系
机译:球状星团中两个不同的蓝色散射星序列 m30
机译:二元二元碰撞涉及主序星,白矮星和球状星团中的中子星。