Spectra of X-ray galaxies in filaments
Large-scale structure of Universe consists of galaxy clusters connected by filaments. Single filaments can be detected at redshifts up to 0.15. The general characteriscis of X-ray spectra of Sloan Digital Sky Survey galaxies, that lies outside clusters, are considered in this work. Seyfert 1 AGN...
Main Author: | A. V Tugay |
---|---|
Format: | Article |
Language: | English |
Published: |
National Aviation University
2013-10-01
|
Series: | Вісник Астрономічної школи |
Subjects: | |
Online Access: | http://astro.nau.edu.ua/issues/2013_V.9_Iss.1/Tugay.html |
Similar Items
-
Dark matter filaments
by: A. V. Tugay
Published: (2018-12-01) -
Observations of interacting galaxies NGC 2341 and NGC 2342 in X-ray band
by: A. V. Tugay, et al.
Published: (2018-12-01) -
X-ray emission of galaxies with emission lines
by: A. V. Tugay, et al.
Published: (2011-10-01) -
Filaments of galaxies and Voronoi diagrams
by: Zaninetti Lorenzo
Published: (2018-12-01) -
The Galaxy–Halo Connection of DESI Luminous Red Galaxies with Subhalo Abundance Matching
by: Angela M. Berti, et al.
Published: (2023-01-01)