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The Morphology–Density Relationship in 1 < z < 2 Clusters
The Astrophysical Journal ( IF 4.8 ) Pub Date : 2020-08-14 , DOI: 10.3847/1538-4357/aba42f
Elizaveta Sazonova 1 , Katherine Alatalo 1, 2 , Jennifer Lotz 2, 3 , Kate Rowlands 1, 2 , Gregory F. Snyder 2 , Kyle Boone 4 , Mark Brodwin 5 , Brian Hayden 4 , Lauranne Lanz 6 , Saul Perlmutter 4 , Vicente Rodriguez-Gomez 7
Affiliation  

The morphology-density relationship states that dense cosmic environments such as galaxy clusters have an overabundance of quiescent elliptical galaxies, but it is unclear at which redshift this relationship is first established. We study the morphology of 4 clusters with $1.2

中文翻译:

1 < z < 2 个簇中的形态-密度关系

形态密度关系表明,稠密的宇宙环境(如星系团)有过多的静止椭圆星系,但尚不清楚这种关系是在哪个红移处首次建立的。我们用 $1.2 研究 4 个簇的形态
更新日期:2020-08-14
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