Statements (60)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:astronomy
|
| gptkbp:are_found_around |
gptkb:Black_holes
gptkb:Neutron_stars Young stars |
| gptkbp:are_theoretical_models_for |
gptkb:Active_galactic_nuclei
Quasars Gamma-ray bursts |
| gptkbp:can_be_found_in |
gptkb:Supermassive_black_holes
Protoplanetary disks X-ray binaries Accreting white dwarfs |
| gptkbp:can_create |
Interstellar medium
Material from companion stars |
| gptkbp:can_lead_to |
Supernovae
Gravitational waves Chemical enrichment Planet formation Jet formation |
| gptkbp:consists_of |
gptkb:natural_gas
gptkb:Dust |
| gptkbp:emissions_standard |
gptkb:X-rays
Radio waves |
| gptkbp:exhibits |
Instabilities
Magnetorotational instability Thermal instability |
| gptkbp:financial_stability |
Viscous forces
Magnetic forces |
| https://www.w3.org/2000/01/rdf-schema#label |
Accretion Disks
|
| gptkbp:influence |
Galaxy morphology
Star formation rates |
| gptkbp:is_affected_by |
Tidal forces
Gravitational interactions Radiation pressure Accretion rate |
| gptkbp:is_analyzed_in |
gptkb:spectroscopy
Numerical simulations |
| gptkbp:is_associated_with |
High-energy astrophysics
|
| gptkbp:is_characterized_by |
Angular momentum
Temperature gradients |
| gptkbp:is_described_as |
gptkb:Navier-Stokes_equations
Hydrodynamics Magnetohydrodynamics |
| gptkbp:is_essential_for |
Galaxy evolution
Star formation Astrophysical jets |
| gptkbp:is_influenced_by |
Magnetic fields
|
| gptkbp:is_observed_in |
Galaxies
Binary star systems |
| gptkbp:is_related_to |
Accretion processes
|
| gptkbp:is_studied_in |
gptkb:astronomy
Theoretical models Observational astronomy Gravitational lensing Time-domain astronomy |
| gptkbp:is_subject_to |
Radiative processes
|
| gptkbp:key |
Cosmic evolution
Black hole growth Energy output of galaxies |
| gptkbp:bfsParent |
gptkb:Black_Holes
|
| gptkbp:bfsLayer |
4
|