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首页> 外文期刊>Astrophysics >Groups of galaxies. IV. Effect of observational selection on the relationship between the characteristics and distance of groups and a comparison with the groups of Geller and Huchra
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Groups of galaxies. IV. Effect of observational selection on the relationship between the characteristics and distance of groups and a comparison with the groups of Geller and Huchra

机译:星系组。 IV。观察选择对群体特征与距离之间关系的影响以及与盖勒和赫赫拉群体的比较

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摘要

The effect of observational selection on the relationship between the characteristics of groups of galaxies and their distances is discussed in this paper. For our groups the dependence of the pairwise distance between the members on the distance of the group is just that. For the groups of Geller and Huchra, on the other hand, the analogous dependence is distorted by the effect of their selection criteria for groups of galaxies. The average dispersion of the radial velocities of the galaxies for our groups is less than half that for the groups of Geller and Huchra, while the mass-to-luminosity ratio is smaller, on the average, by more than an order of magnitude in our case. Geller-Huchra groups with mass-to-luminosity ratios greater than 1000 are most likely unreal.
机译:本文讨论了观测选择对星系组特征与其距离之间关系的影响。对于我们的组,成员之间的成对距离对组距离的依赖性就是这样。另一方面,对于盖勒(Geller)和霍赫拉(Huchra)组,类似的依赖性因其对星系组选择标准的影响而失真。我们各组的星系径向速度的平均分散度小于盖勒和赫赫拉各组的一半,而质量与光度之比平均更小,超过了我们案件。质量流明比大于1000的Geller-Huchra组很可能是不真实的。

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