Study of Substructures in SDSS Supercluster S[173+014+0082]

Authors

  • Janak Ratna Malla Amrit Campus, Department of Physics, Tribhuvan University, Kathmandu, Nepal
  • Walter Saurer Institute of Astroparticle Physics Innsbruck University, Technistrasse 25/8, Innsbruck, Austria
  • Binil Aryal Central Department of Physics Tribhuvan University, Kirtipur, Nepal

DOI:

https://doi.org/10.3126/jnphyssoc.v8i1.48283

Keywords:

Galaxies, evolution galaxies, superclusters galaxies, statistics

Abstract

We present magnitude, color, redshift and number density distributions of 1302 galaxies in the supercluster S[173+014+0082]. Our aim is to identify substructures and study their redshift maps. The visual magnitude distribution suggests that the supercluster is dynamically unstable. We found 3 substructures in the supercluster region having mean redshift 0.083, 0.085 and 0.090. An empirical relation be-tween the number of galaxies in the substructures and their mean redshift is observed.

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Published

2022-12-13

How to Cite

Malla, J. R., Saurer, W., & Aryal, B. (2022). Study of Substructures in SDSS Supercluster S[173+014+0082]. Journal of Nepal Physical Society, 8(1), 35–38. https://doi.org/10.3126/jnphyssoc.v8i1.48283

Issue

Vol. 8 No. 1 (2022): ICFP JNPS Special Issue

Section

Articles

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