Statements (55)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
gptkb:observatory
|
| gptkbp:area |
Magnetic fields
Angular momentum |
| gptkbp:canBe |
Radiation pressure
Viscous heating |
| gptkbp:canEstablish |
X-rays
Turbulence Radio waves Differential rotation Visible light |
| gptkbp:canLeadTo |
Tidal forces
Gravitational waves Instabilities Planet formation Accretion onto central object Disk instabilities Jet formation |
| gptkbp:formFactor |
Black holes
Young stars Neutron stars |
| gptkbp:hasInfluenceOn |
Surrounding environment
Star formation rates Galaxy dynamics |
| https://www.w3.org/2000/01/rdf-schema#label |
Accretion Disks
|
| gptkbp:isCharacterizedBy |
High temperatures
High densities |
| gptkbp:isComposedOf |
Gas
Dust |
| gptkbp:isCounteredBy |
Magnetic fields
Numerical simulations Computational models Hydrodynamic simulations Magnetohydrodynamic simulations Self-gravity |
| gptkbp:isFoundIn |
Galaxies
Star clusters |
| gptkbp:isImportantFor |
Star formation
Galaxy formation |
| gptkbp:isRelatedTo |
gptkb:Supernova_remnants
Quasars Gamma-ray bursts |
| gptkbp:isStudiedIn |
Astrophysics
Cosmology |
| gptkbp:isUsedFor |
gptkb:Kepler's_laws
Hydrodynamics Magnetohydrodynamics Active galactic nuclei X-ray binaries Navier-Stokes_equations Protoplanetary_disks |
| gptkbp:isUtilizedFor |
Astrophysical jets
Accretion processes. |
| gptkbp:keyIssues |
Understanding stellar evolution
Understanding galaxy evolution Understanding black hole growth |