机译:内外开放恒星团内行星的频率相同
Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA;
Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA;
Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA;
Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA;
NASA Ames Research Center, Moffett Field, California 94035, USA;
NASA Exoplanet Science Institute, California Institute of Technology, Pasadena, California 91125, USA;
NASA Ames Research Center, Moffett Field, California 94035, USA;
California Institute of Technology, Pasadena, California 91125, USA;
NASA Ames Research Center, Moffett Field, California 94035, USA;
Boston University, Boston, Massachusetts 02215, USA;
Leibniz-lnstitute for Astrophysics, Potsdam 14467, Germany,Space Science Institute, Boulder, Colorado 80301, USA;
University of California, Berkeley, Berkeley, California 94720, USA;
University of California, Berkeley, Berkeley, California 94720, USA;
Yale University, New Haven,Connecticut 06520, USA;
NASA Ames Research Center, Moffett Field, California 94035, USA;
Southern Connecticut State University, New Haven, Connecticut 06515, USA;
SEN Institute/NASA Ames Research Center, Moffett Field, California 94035, USA;
National Optical Astronomy Observatory, Tucson, Arizona 85719, USA;
University of Notre Dame, Notre Dame, Indiana 46556, USA;
机译:密集的恒星团内部的行星形成
机译:恒星群中的行星广泛搜索。 V.在旧的开放星团NGC 188中搜寻行星并识别18个新的变星。
机译:广泛间隔的行星宿主恒星的双频-行星宿主恒星的新棕矮星伴星
机译:Gemini Nici Planet-Printing Campaign:年轻B和星星周围的巨型行星频率
机译:连接点:通过观察恒星,圆盘和行星中的碳和氧物种,研究行星的形成和组成。
机译:遥远的生命探测标准可居住的区域边界以及M星和K晚星周围类似地球的行星的频率
机译:内外开放恒星团内行星的频率相同
机译:从星星到超行星:年轻星团IC348中的低质量ImF