机译:NGC 5253中高效的恒星形成,可能是由流加料产生的
Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, California 90095-1547, USA;
Department of Physics and Astronomy, University of Tel Aviv, 69978 Ramat Aviv, Israel;
Observational Cosmology Laboratory, Code 665, NASA at Goddard Space Flight Center, Greenbelt, Maryland 20771, USA;
Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, California 90095-1547, USA;
Academia Sinica, Astronomy and Astrophysics, 11F Astronomy-Mathematics Building, AS/NTU No. 1,Sec.4, Roosevelt Road, Taipei 10617, Taiwan;
Department of Physics, Caltech, Pasadena, California 91125, USA, Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55405, USA;
Department of Physics, New Mexico Institute of Mining and Technology, Socorro, New Mexico 85723, USA,National Radio Astronomy Observatory, 1003 Lopezville Road, Socorro, New Mexico 85723, USA;
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA;
机译:NGC 5253和NGC 3077的最新集群形成历史:对恒星形成的环境影响
机译:NGC 5253和NGC 3077的最近星团形成历史:环境对恒星形成的影响*
机译:NGC 5253和NGC 3077的最新集群形成历史:对恒星形成的环境影响
机译:NGC 5253中核星团核心群的大规模恒星含量
机译:IRAS明亮早期型星系的星际中和恒星形成:NGC 3032,NGC 3928,NGC 7465和NGC 7625
机译:实验室对年轻恒星积聚物质的研究
机译:NGC 5253中高效的恒星形成,可能是由流加料产生的