Statements (59)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
Molecular Cloud
|
| gptkbp:associated_with |
Star Clusters
H II Regions |
| gptkbp:can_be |
Stars
Shock Waves |
| gptkbp:composedOf |
Hydrogen
|
| gptkbp:contains |
Gas
Dust |
| gptkbp:contributedTo |
Galactic_Chemical_Enrichment
|
| gptkbp:features |
Astrobiology_Research
|
| gptkbp:has_a |
50 to 600 light-years
|
| https://www.w3.org/2000/01/rdf-schema#label |
Giant Molecular Cloud
|
| gptkbp:impact |
Radiation Pressure
Galactic_Dynamics |
| gptkbp:includes |
Complex_Organic_Molecules
|
| gptkbp:influenced |
Turbulence
Magnetic Fields Supernova Explosions Galactic_Winds |
| gptkbp:is_a |
gptkb:Globular_Clusters
|
| gptkbp:is_a_key_component_of |
Star Formation Theory
|
| gptkbp:is_a_site_for |
Planet Formation
Massive Star Formation Chemical_Complexity |
| gptkbp:is_a_source_of |
gptkb:Molecular_Hydrogen
gptkb:Cosmic_Rays Star Formation Regions Interstellar Water Prestellar_Cores |
| gptkbp:is_available_in |
gptkb:Starburst_Galaxies
Galaxies The Milky Way Nearby Galaxies |
| gptkbp:is_characterized_by |
High Density
Low Temperature |
| gptkbp:is_essential_for |
Galaxy_Evolution
|
| gptkbp:is_featured_in |
gptkb:Spiral_Galaxies
Star-Forming Regions |
| gptkbp:is_located_in |
gptkb:Supernova_Remnants
|
| gptkbp:is_monitored_by |
Submillimeter_Astronomy
|
| gptkbp:is_part_of |
Interstellar Medium
Giant_Molecular_Associations |
| gptkbp:is_popular_among |
Heavy Elements
Optical Wavelengths 3D_Space |
| gptkbp:is_studied_in |
Astrophysics
Radio Astronomy Galaxy Formation Chemical Evolution Star Formation Rates Star_Cluster_Formation |
| gptkbp:is_used_in |
Spectroscopy
Dark Nebulae Molecular Outflows Molecular_Line_Observations |
| gptkbp:region |
Star Formation
|
| gptkbp:visitedBy |
Infrared
CO_Emission_Lines |
| gptkbp:was_a_factor_in |
Galaxy_Dynamics
|