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,
Н.Ш. Алимгазинова,
A.M. Demesinova,
U.Zh. Sagyntayeva,
A.B. Manapbayeva,
A. K. Kuratova,
A. Zh. Naurzbaeva,
М.Т. Кызгарина
Publication year - 2020
Publication title -
recent contributions to physics
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
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom