The SAMI Galaxy Survey: Data Release Two with absorption-line physics value-added products

The SAMI Galaxy Survey: Data Release Two with absorption-line physics value-added products
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DOI:
10.1093/mnras/sty2355
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发表时间:
2018-08
影响因子:
4.8
通讯作者:
N. Scott;J. van de Sande-J.-van de Sande-2124254137;S. Croom;B. Groves;M. Owers;H. Poetrodjojo;F. d’Eugenio;A. Medling;D. Barat;T. Barone;J. Bland-Hawthorn;S. Brough;J. Bryant;L. Cortese;C. Foster;A. Green;Sree Oh;M. Colless;M. Drinkwater;S. Driver;M. Goodwin;M. Gunawardhana;C. Federrath;L. Harischandra;Yifei Jin;J. Lawrence;N. Lorente;E. Mannering;S. O’Toole;S. Richards;S. Sánchez;A. Schaefer;K. Sealey;R. Sharp;S. Sweet;D. Taranu;Mathew R Varidel
N. Scott;J. van de Sande-J.-van de Sande-2124254137;S. Croom;B. Groves;M. Owers;H. Poetrodjojo;F. d’Eugenio;A. Medling;D. Barat;T. Barone;J. Bland-Hawthorn;S. Brough;J. Bryant;L. Cortese;C. Foster;A. Green;Sree Oh;M. Colless;M. Drinkwater;S. Driver;M. Goodwin;M. Gunawardhana;C. Federrath;L. Harischandra;Yifei Jin;J. Lawrence;N. Lorente;E. Mannering;S. O’Toole;S. Richards;S. Sánchez;A. Schaefer;K. Sealey;R. Sharp;S. Sweet;D. Taranu;Mathew R Varidel
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
N. Scott;J. van de Sande-J.-van de Sande-2124254137;S. Croom;B. Groves;M. Owers;H. Poetrodjojo;F. d’Eugenio;A. Medling;D. Barat;T. Barone;J. Bland-Hawthorn;S. Brough;J. Bryant;L. Cortese;C. Foster;A. Green;Sree Oh;M. Colless;M. Drinkwater;S. Driver;M. Goodwin;M. Gunawardhana;C. Federrath;L. Harischandra;Yifei Jin;J. Lawrence;N. Lorente;E. Mannering;S. O’Toole;S. Richards;S. Sánchez;A. Schaefer;K. Sealey;R. Sharp;S. Sweet;D. Taranu;Mathew R Varidel

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我们目前的第二个主要发布的数据从悉尼-澳大利亚天文台多目标积分场摄谱仪(SAMI)星系调查。数据发布二包括1559个星系的数据,约占全部调查的50%。包括Galerkin的红移范围为0.004 [11],速度色散向中心强烈增加,而低于log(M-*/M-圆点)< 10,我们没有发现中心速度色散明显增加的证据。这表明,对于有或没有弥散主导的凸起的星系,log(M */M圆点)附近的过渡质量类似于10。
We present the second major release of data from the Sydney - Australian Astronomical Observatory Multi-Object Integral Field Spectrograph (SAMI) Galaxy Survey. Data Release Two includes data for 1559 galaxies, about 50 per cent of the full survey. Galaxies included have a redshift range 0.004 11], the velocity dispersion strongly increases towards the centre, whereas below log (M-*/M-circle dot) < 10 we find no evidence for a clear increase in the central velocity dispersion. This suggests a transition mass around log (M-*/M-circle dot) similar to 10 for galaxies with or without a dispersion-dominated bulge.