Description: Symmetries and Dynamics of Star Clusters Please note: this item is printed on demand and will take extra time before it can be dispatched to you (up to 20 working days). Author(s): Jaroslav Haas Format: Paperback Publisher: Springer International Publishing AG, Switzerland Imprint: Springer International Publishing AG ISBN-13: 9783319378572, 978-3319378572 Synopsis In this PhD thesis, which was nominated for publication in this series by the Astronomical Institute at Charles University, Prague, the author investigates the orbital evolution of an initially thin stellar disc around a supermassive black hole, considering various perturbative sources of gravity. His findings, obtained by both direct numerical N-body modelling and using standard perturbation methods, offer a viable theoretical explanation for the observed configuration of young stars in the Galactic Centre. This marks a significant contribution to a topic of great interest in contemporary astrophysics. The author also shows in his thesis that a secular instability (m = 1 mode) may occur in the embedding spherical cluster of old stars. This increases the richness of possible evolution scenarios of the embedding cluster and may lead to effective feeding of supermassive black holes through tidal disruption of stars on extremely eccentric orbits.
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Book Title: Symmetries and Dynamics of Star Clusters
Number of Pages: 79 Pages
Language: English
Publication Name: Symmetries and Dynamics of Star Clusters
Publisher: Springer International Publishing A&G
Publication Year: 2016
Subject: Physics
Item Height: 235 mm
Item Weight: 1591 g
Type: Textbook
Author: Jaroslav Haas
Series: Springer Theses
Item Width: 155 mm
Format: Paperback