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机译:与其伴侣恒星星系相比,没有证据增强[oiii]88μm排放88μm发射
Max Planck Institute for Astronomy K?nigstuhl 17 D-69117 Heidelberg Germany;
Cornell University 220 Space Sciences Building Ithaca NY 14853 USA;
Max Planck Institute for Astronomy K?nigstuhl 17 D-69117 Heidelberg Germany;
INAF Osservatorio di Astrofisica e Scienza dello Spazio via Gobetti 93/3 I-40129 Bologna Italy;
Winona State University Winona MN 55987 USA;
Max Planck Institute for Astronomy K?nigstuhl 17 D-69117 Heidelberg Germany;
The Observatories of the Carnegie Institution for Science 813 Santa Barbara Street Pasadena CA 91101 USA;
Argelander-Institut für Astronomie Universit?t Bonn Auf dem Hügel 71 D-53121 Bonn Germany;
National Radio Astronomy Observatory Pete V. Domenici Array Science Center P.O. Box O Socorro NM 87801 USA;
Steward Observatory The University of Arizona 933 North Cherry Avenue Tucson AZ 85721 USA;
University of California Santa Barbara Santa Barbara CA USA;
European Southern Observatory Alonso de Córdova 3107 Vitacura Región Metropolitana Chile;
Max Planck Institute for Astronomy K?nigstuhl 17 D-69117 Heidelberg Germany;
Max Planck Institute for Astronomy K?nigstuhl 17 D-69117 Heidelberg Germany;
Department of Astrophysical Sciences Princeton University Princeton NJ 08544 USA;
National Radio Astronomy Observatory Pete V. Domenici Array Science Center P.O. Box O Socorro NM 87801 USA;
Kavli Institute of Astronomy and Astrophysics at Peking University No.5 Yiheyuan Road Haidian District Beijing 100871 People?s Republic of China;
high-redshift; galaxies: ISM; quasars: emission lines; quasars: general; submillimeter: ISM;
机译:与其伴侣恒星星系相比,没有证据增强[oiii]88μm排放88μm发射
机译:大三龙:z = 7.15莱曼 - 中断的星系,在[oiii] 88 mu m,[cii] 158 mu m,以及与阿尔玛的灰尘连续
机译:与大规模星系相比,极大规模类星体不是密集环境的良好代理:极大规模类星体和星系的环境
机译:PG Quasars中的发射线谱
机译:QSO宿主星系和伴星中相互作用引起的星爆的年龄定年。
机译:从内星系的漫射光发射线发现:Li(n)r样气的证据
机译:没有证据于Z〜6 Quasar的增强型O III88μm排放,而与其伴侣恒星的星系相比