Position Angle Distribution of Galaxies in 35 Cluster

Authors

  • Shiv Narayan Yadav Central Department of Phhysics, Tribhuvan University, Kirtipur
  • Binil Aryal Central Department of Phhysics, Tribhuvan University, Kirtipur
  • Walter Saurer Institute of Astro-particle Physics, Innsbruck University, Innsbruck

DOI:

https://doi.org/10.3126/hj.v4i0.9417

Keywords:

Galaxies, Evolution, Formation, Statistics, Clusters, General

Abstract

We worked on POSSII and ESO films and measured the diameters and position angles of 5 688 galaxies in 34 clusters using 25-fold magnification microscope. The position angle distributions of galaxies in the clusters are studied. For this, chi-square, auto-correlation and the Fourier tests are carried out. The preferred position angle distribution of galaxies in the cluster is found to be independent of the mean radial velocity of the cluster. Possible explanations of the result will be discussed.

The Himalayan Physics

Vol. 4, No. 4, 2013

Page: 1-9

Uploaded date: 12/22/2013

 

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Published

2013-12-22

How to Cite

Yadav, S. N., Aryal, B., & Saurer, W. (2013). Position Angle Distribution of Galaxies in 35 Cluster. Himalayan Physics, 4, 1–9. https://doi.org/10.3126/hj.v4i0.9417

Issue

Vol. 4 (2013)

Section

Articles

License

The articles published in the Himalayan Physics are distributed under a license CC BY-NC-SA 4.0.