Statements (107)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:astronomy
|
| gptkbp:contains |
gptkb:supermassive_black_hole
gptkb:Sagittarius_A* young stars |
| gptkbp:has_a_focus_on |
public interest
theoretical astrophysics astrophysical research |
| gptkbp:has_a_supermassive_black_hole |
gptkb:Sagittarius_A*
|
| gptkbp:has_high_energy |
cosmic rays
|
| https://www.w3.org/2000/01/rdf-schema#label |
Galactic Center
|
| gptkbp:is_a |
gptkb:region
|
| gptkbp:is_a_focal_point_for |
the Milky Way's structure
|
| gptkbp:is_a_site_of |
black hole studies
star formation accretion processes massive star clusters cosmic interactions |
| gptkbp:is_a_source_of |
gptkb:X-rays
gptkb:gravitational_waves radio waves stellar winds stellar flares |
| gptkbp:is_a_subject_of |
scientific inquiry
theoretical models |
| gptkbp:is_affected_by |
magnetic fields
supernovae stellar winds |
| gptkbp:is_approximately |
26,000 light-years from Earth
|
| gptkbp:is_associated_with |
gptkb:Sagittarius_A*
gptkb:supernova_remnants star formation black hole physics gamma-ray emissions stellar remnants |
| gptkbp:is_characterized_by |
high luminosity
high stellar density high-energy phenomena high density of gas |
| gptkbp:is_connected_to |
gptkb:Galactic_bulge
galactic evolution galactic rotation |
| gptkbp:is_explored_in |
gptkb:spectroscopy
space telescopes X-ray observations |
| gptkbp:is_home_to |
gptkb:interstellar_medium
young stars massive stars various types of stars massive black holes |
| gptkbp:is_influenced_by |
gptkb:dark_matter
stellar evolution galactic winds |
| gptkbp:is_involved_in |
galactic dynamics
|
| gptkbp:is_linked_to |
galactic dynamics
galactic evolution stellar populations galactic interactions |
| gptkbp:is_located_in |
gptkb:Milky_Way_Galaxy
stellar nurseries stellar collisions |
| gptkbp:is_monitored_by |
observatories
|
| gptkbp:is_near |
star clusters
|
| gptkbp:is_observed_in |
gptkb:space_mission
multiple wavelengths |
| gptkbp:is_part_of |
gptkb:Galactic_Halo
gptkb:Galactic_core gptkb:the_Local_Group Milky Way structure the Galactic bulge Galactic nucleus the Galactic halo the Galactic core |
| gptkbp:is_studied_for |
gptkb:cosmology
black hole activity |
| gptkbp:is_studied_in |
gptkb:astronomy
infrared telescopes radio telescopes |
| gptkbp:is_subject_to |
gravitational forces
|
| gptkbp:is_surrounded_by |
gptkb:star
molecular clouds stellar nurseries dark clouds gas clouds dense star clusters |
| gptkbp:is_visible_from |
gptkb:Earth
infrared wavelengths |
| gptkbp:located_in |
gptkb:Milky_Way_Galaxy
|
| gptkbp:map |
astrophysicists
space telescopes infrared surveys |
| gptkbp:mass |
4.1 million solar masses
|
| gptkbp:region |
gptkb:active_galactic_nuclei
high metallicity intense radiation extreme gravitational forces high stellar density high stellar activity high angular momentum high temperature gas high density gas high cosmic ray activity |
| gptkbp:targets |
future missions
observational campaigns |
| gptkbp:bfsParent |
gptkb:Centaurus
gptkb:The_Sun gptkb:Milky_Way |
| gptkbp:bfsLayer |
5
|