z-logo
open-access-imgOpen Access
Description of the scenario for the development of proto galaxies with small angular momentum through cascade fragmentation with the formation of proto clusters and proto stars based on graph theory
Author(s) -
A.T. Mailybaev,
V. A. Zakhozhay,
N.Sh. Alimgazinova,
Aziza Demesinova,
U.Zh. Sagyntayeva,
A.B. Manapbayeva,
A. K. Kuratova,
A. Zh. Naurzbaeva,
M.T. Kyzgarina
Publication year - 2020
Publication title -
vestnik. seriâ fizičeskaâ/habaršysy - a̋l-farabi atyndaġy k̦azak̦ memlekettik u̇lttyk̦ universitetì. fizika seriâsy
Language(s) - English
Resource type - Journals
eISSN - 2663-2276
pISSN - 1563-0315
DOI - 10.26577/rcph.2020.v72.i1.04
Subject(s) - physics , astrophysics , stars , star formation , initial mass function , galaxy , fragmentation (computing) , galaxy formation and evolution , stellar mass , cascade , astronomy , chemistry , chromatography , computer science , operating system

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here