机译:银河系盘平面两侧的两个化学相似的恒星密度
Max Planck Inst Astron, Koenigstuhl 17, D-69117 Heidelberg, Germany;
Deutsch Borse AG, Mergenthalerallee 61, D-65760 Eschborn, Germany;
CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA;
CSIC, Inst Space Sci ICE, Carrer Can Magrans, E-08193 Barcelona, Spain;
CUNY, Dept Nat Sci, LaGuardia Community Coll, 31-10 Thomson Ave, Long Isl City, NY 11101 USA;
Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA;
Australian Natl Univ, Res Sch Astron & Astrophys, Mt Stromlo Observ, Canberra, ACT 2611, Australia;
Columbia Univ, Dept Astron, 550 West 120th St,Mail Code 5246, New York, NY 10027 USA;
Columbia Univ, Dept Astron, 550 West 120th St,Mail Code 5246, New York, NY 10027 USA;
Princeton Univ, Dept Astrophys Sci, 4 Ivy Lane, Princeton, NJ 08544 USA;
Univ Oxford, Rudolf Peierls Ctr Theoret Phys, 1 Keble Rd, Oxford OX1 3NP, England;
Max Planck Inst Astron, Koenigstuhl 17, D-69117 Heidelberg, Germany;
机译:银河系飞掠EN击盘的形成。 I.星盘
机译:Monoceros环和A13恒星密度的磁盘起源
机译:SMMCing LMC:在LMC磁盘中映射环状恒星密度
机译:由半乳扁中心的分子云的碰撞形成的年轻恒星盘
机译:活跃银河核中的黑洞和吸积盘:微透镜,焦散和恒星碰撞动力学。
机译:二元合并和恒星崩溃之后的黑洞磁盘和喷流:电磁发光度和吸积率的范围狭窄
机译:银河薄盘和厚盘恒星种群化学演化历史的比较