首页> 外文期刊>The Astrophysical Journal. Letters >SDSS-IV MaNGA: Probing the Kinematic Morphology-Density Relation of Early-type Galaxies with MaNGA
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SDSS-IV MaNGA: Probing the Kinematic Morphology-Density Relation of Early-type Galaxies with MaNGA

机译:SDSS-IV Manga:探讨早期星系与漫画的运动形态密度关系

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摘要

The “kinematic" morphology-density relation for early-type galaxies posits that those galaxies with low angular momentum are preferentially found in the highest-density regions of the universe. We use a large sample of galaxy groups with halo masses 10~(12.5) < M_(halo)< 10~(14.5) h~(-1) M_⊙ observed with the Mapping Nearby Galaxies at APO (MaNGA) survey to examine whether there is a correlation between local environment and rotational support that is independent of stellar mass. We find no compelling evidence for a relationship between the angular momentum content of early-type galaxies and either local overdensity or radial position within the group at fixed stellar mass.
机译:用于早期星系的“运动”形态学 - 密度关系,其中具有低角度动量的星系优先在宇宙的最高密度区域中发现。我们使用晕群10〜(12.5)使用大型银河系样本

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  • 作者单位

    Department of Astrophysics Princeton University Princeton NJ 08540 USA;

    Department of Astronomy and Astrophysics University of California Santa Cruz 1156 High Street Santa Cruz CA 95064 USA;

    European Southern Observatory Karl-Schwarzschild-Str. 2 D-85741 Garching Germany;

    Institute of Cosmology and Gravitation University of Portsmouth Dennis Sciama Building Burnaby Road Portsmouth PO1 3FX UK;

    National Astronomical Observatories Chinese Academy of Sciences 20A Datun Road Chaoyang District Beijing 100012 China;

    PITT PACC Department of Physics and Astronomy University of Pittsburgh Pittsburgh PA 15260 USA;

    Apache Point Observatory P.O. Box 59 sunspot NM 88349 USA;

    Department of Physics and Astronomy University of Utah 115 S. 1400 E. Salt Lake City UT 84112 USA;

    Department of Astrophysics Princeton University Princeton NJ 08540 USA;

    Space Telescope Science Institute 3700 San Martin Drive Baltimore MD 21218 USA;

    Institute of Astronomy and Astrophysics Academia Sinica Taipei 10617 Taiwan;

    Institute of Cosmology and Gravitation University of Portsmouth Dennis Sciama Building Burnaby Road Portsmouth PO1 3FX UK;

    School of Physics and Astronomy The University of Nottingham University Park Nottingham NG7 2RD UK;

    Kavli Institute for the Physics and Mathematics of the Universe (WPI) Tokyo Institutes for Advanced Study The University of Tokyo 5-1-5 Kashiwanoha Kashiwa-shi Chiba 277-8583 Japan;

    Department of Physical Science Hiroshima University 1-3-1 Kagamiyama Higashi-Hiroshima Hiroshima 739-8526 Japan;

    Department of Astronomy and Astrophysics The Pennsylvania State University University Park PA 16802 USA;

    Institute of Cosmology and Gravitation University of Portsmouth Dennis Sciama Building Burnaby Road Portsmouth PO1 3FX UK;

    School of Physical Sciences The Open University Milton Keynes MK7 6AA UK;

    Department of Physics and Astronomy University of Kentucky 505 Rose Street Lexington KY 40506-0057 USA;

    McDonald Observatory The University of Texas at Austin 1 University Station Austin TX 78712 USA;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天体力学(理论天文学);
  • 关键词

    galaxies: elliptical and lenticular; cD; galaxies: groups: general; galaxies: kinematics and dynamics;

    机译:星系:椭圆形和透镜;CD;星系:团体:一般;Galaxies:Kinematics和Dynamics;

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