Statements (70)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:age |
few million years
|
| gptkbp:contains |
gptkb:30_Doradus
star-forming regions nebulae massive stars young massive clusters |
| gptkbp:distance_from_earth |
163,000 light years
|
| gptkbp:features |
massive star formation
|
| gptkbp:has_high_star_formation_rate |
gptkb:true
|
| https://www.w3.org/2000/01/rdf-schema#label |
LMC star formation region
|
| gptkbp:is_affected_by |
radiation pressure
galactic winds galactic turbulence |
| gptkbp:is_associated_with |
gptkb:dark_matter
gptkb:supernova_remnants star clusters stellar winds stellar nurseries |
| gptkbp:is_characterized_by |
molecular clouds
high metallicity HII regions stellar feedback stellar mergers massive star formation events stellar outflows high density regions |
| gptkbp:is_home_to |
gptkb:Wolf-Rayet_stars
young stellar objects massive star clusters red supergiants open clusters stellar associations massive stellar populations massive protostars |
| gptkbp:is_influenced_by |
gptkb:interstellar_medium
cosmic rays supernova explosions galactic interactions |
| gptkbp:is_known_for |
active star formation
bright emission lines high stellar density high star formation efficiency |
| gptkbp:is_observed_in |
infrared wavelengths
|
| gptkbp:is_part_of |
gptkb:galaxy
gptkb:Ring_of_Honor gptkb:LMC gptkb:star star formation activity star formation history intergalactic medium cosmic web star formation network |
| gptkbp:is_studied_for |
stellar evolution
galactic evolution star formation processes stellar population synthesis chemical enrichment dynamics of star formation interstellar chemistry |
| gptkbp:is_studied_in |
gptkb:astronomy
|
| gptkbp:is_visible_from |
gptkb:Earth
optical wavelengths X-ray wavelengths radio wavelengths ultraviolet wavelengths |
| gptkbp:located_in |
gptkb:Large_Magellanic_Cloud
|
| gptkbp:bfsParent |
gptkb:NGC_2004
gptkb:Supernova_remnant_1987_A |
| gptkbp:bfsLayer |
6
|