Spatial orientation of angular momentum vectors of galaxies in six rotating clusters
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/434/3/1939/18495815/stt1124.pdf
Reference61 articles.
1. A catalog of rich clusters of galaxies
2. Spin vector orientations of galaxies in eight Abell clusters of BM type I
3. Spin vector orientation of galaxies in the region 15h 48m≤α(2000) ≤ 19h 28m, −68°≤δ(2000) ≤−62°
4. Spatial orientations of galaxies in 10 Abell clusters of BM type II-III
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1. Galaxy Cluster Mass Estimates in the Presence of Substructure;The Astrophysical Journal;2020-01-15
2. Investigation of the orientation of galaxies in clusters: the importance, methods and results of research;Journal of Cosmology and Astroparticle Physics;2019-02-05
3. The non-Gaussian distribution of galaxy gravitational fields;Research in Astronomy and Astrophysics;2017-12
4. Preferred alignments of angular momentum vectors of galaxies in six dynamically unstable Abell clusters;Research in Astronomy and Astrophysics;2017-07
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