Statements (54)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:bfsLayer |
5
|
| gptkbp:bfsParent |
gptkb:NGC_1866
|
| gptkbp:age |
a few million years
|
| gptkbp:contains |
gptkb:NGC_2070
gptkb:30_Doradus |
| gptkbp:depicted_in |
gptkb:physicist
optical wavelengths radio wavelengths |
| gptkbp:distance |
approximately 163,000 light years
|
| gptkbp:examines |
astrophysicists
space telescopes ground-based telescopes |
| https://www.w3.org/2000/01/rdf-schema#label |
LMC star forming complex
|
| gptkbp:is_affected_by |
metallicity variations
|
| gptkbp:is_associated_with |
gptkb:supernova_remnants
star clusters stellar nurseries massive star clusters stellar feedback interstellar shocks |
| gptkbp:is_characterized_by |
molecular clouds
stellar outflows high star formation rate high density gas star formation bursts |
| gptkbp:is_connected_to |
galactic interactions
dark matter halo star formation theories |
| gptkbp:is_home_to |
massive star formation
young stellar objects massive stars HII regions OB associations pre-main sequence stars |
| gptkbp:is_influenced_by |
environmental factors
cosmic rays galactic winds |
| gptkbp:is_observed_in |
infrared wavelengths
|
| gptkbp:is_part_of |
gptkb:interstellar_medium
gptkb:LMC cosmic web LMC galaxy star forming complexes |
| gptkbp:is_studied_in |
gptkb:observatory
galactic dynamics stellar evolution galactic evolution star formation history chemical enrichment |
| gptkbp:located_in |
gptkb:Large_Magellanic_Cloud
|
| gptkbp:notable_for |
high luminosity
starburst activity bright nebulae |