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Velocity Dispersions and Dynamical Masses for a Large Sample of Quiescent Galaxies at z > 1: Improved Measures of the Growth in Mass and Size

机译：大样本的速度色散和动态质量 z> 1时的静止星系：改进了质量和尺寸增长的测量方法

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Belli, Sirio; Newman, Andrew B.; Ellis, Richard S.;
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年度 2014
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正文语种 {"code":"en","name":"English","id":9}
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1. VELOCITY DISPERSIONS AND DYNAMICAL MASSES FOR A LARGE SAMPLE OF QUIESCENT GALAXIES AT z 1: IMPROVED MEASURES OF THE GROWTH IN MASS AND SIZE [J] . Sirio Belli1, Andrew B. Newman12, Richard S. Ellis1 The Astrophysical journal . 2014,第2期

机译：z> 1时大量大量星系样本的速度色散和动力学质量：质量和尺寸增长的改进措施
2. THE STELLAR VELOCITY DISPERSION OF A COMPACT MASSIVE GALAXY AT z = 1.80 USING X-SHOOTER: CONFIRMATION OF THE EVOLUTION IN THE MASS–SIZE AND MASS–DISPERSION RELATIONS [J] . Jesse van de Sande, Mariska Kriek, Marijn Franx, The Astrophysical Journal. Letters . 2011,第1期

机译：使用X轴在z = 1.80的紧凑型大规模星系的星速散度：证实了质量尺寸和质散关系的演化
3. A STELLAR VELOCITY DISPERSION FOR A STRONGLY LENSED, INTERMEDIATE-MASS QUIESCENT GALAXY AT z = 2.8 [J] . Allison. R. Hill1, Adam Muzzin2, Marijn Franx1, The Astrophysical journal . 2016,第1期

机译：在z = 2.8时强透镜，中间质量银河系的星速色散
4. Galaxy and Mass Assembly (GAMA): galaxy pairwise velocity dispersion [C] . Jon Loveday, Leonidas Christodoulou, the GAMA team International Astronomical Union., Symposium . 2016

机译：星系和大规模组装（GAMA）：Galaxy成对速度分散
5. Dynamical mass modeling of dispersion-supported dwarf galaxies. [D] . Wolf, Joseph. 2011

机译：弥散支持的矮星系的动力学质量建模。
6. Investigation of Dry Powder Inhaler (DPI) Resistance and Aerosol Dispersion Timing on Emitted Aerosol Aerodynamic Particle Sizing by Multistage Cascade Impactor when Sampled Volume Is Reduced from Compendial Value of 4 L [O] . Hlack Mohammed, Jan Arp, Frank Chambers, 2014

机译：当样本量从4 L的标准值减小时多级级联撞击器对干粉吸入器（DPI）的抵抗力和气溶胶分散时间的研究
7. Velocity Dispersions and Dynamical Masses for a Large Sample of Quiescent Galaxies at z > 1: Improved Measures of the Growth in Mass and Size [O] . Belli Sirio, Newman Andrew B., Ellis Richard S. 2014

机译：z> 1时大量静态星系的速度色散和动态质量：质量和尺寸增长的改进度量

Velocity Dispersions and Dynamical Masses for a Large Sample of Quiescent Galaxies at z > 1: Improved Measures of the Growth in Mass and Size

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