STABILITY OF STELLAR SYSTEMS ORBITING SGR A*
Path equations of different orbiting objects in the presence of very strong gravitational fields are essential to examine the impact of its gravitational effect on the stability of each system. Implementing an analogous method, used to examine the stability of planetary systems by solving the geodes...
Main Author: | Magd E. Kahil |
---|---|
Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2016-06-01
|
Series: | Odessa Astronomical Publications |
Subjects: | |
Online Access: | http://oap.onu.edu.ua/article/view/70600 |
Similar Items
-
Resolved SPLASH Chemodynamics in Andromeda’s PHAT Stellar Halo and Disk: On the Nature of the Inner Halo along the Major Axis
by: Ivanna Escala, et al.
Published: (2023-01-01) -
Nonextensive Behavior of Stellar Rotation in the Galactic Disk Components
by: M. P. da Silva, et al.
Published: (2023-01-01) -
Properties of Stellar Streams in the Galactic Disk
by: Marsakov V. A., et al.
Published: (2016-12-01) -
Origins of the Evil Eye: M64's Stellar Halo Reveals the Recent Accretion of an SMC-mass Satellite
by: Adam Smercina, et al.
Published: (2023-01-01) -
Resolved Stellar Mass Estimation of Nearby Late-type Galaxies for the SPHEREx Era: Dependence on Stellar Population Synthesis Models
by: Jeong Hwan Lee, et al.
Published: (2025-01-01)