Statements (46)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:star
|
| gptkbp:are_known_for |
high mass loss rates
high luminosities |
| gptkbp:are_less_common_in |
metal-poor environments
|
| gptkbp:are_part_of |
the evolutionary path of massive stars
the late stages of stellar evolution |
| gptkbp:can_be_found_in |
gptkb:the_Large_Magellanic_Cloud
gptkb:the_Small_Magellanic_Cloud |
| gptkbp:can_detect |
gptkb:spectroscopy
|
| gptkbp:characterized_by |
strong stellar winds
broad emission lines high surface temperatures |
| gptkbp:contribution |
chemical enrichment of the interstellar medium
|
| gptkbp:created |
gptkb:Supernova
black holes |
| gptkbp:emissions_standard |
strong ultraviolet radiation
|
| gptkbp:evolve_from |
massive stars
|
| gptkbp:exhibits |
mass loss rates up to 10^-5 solar masses per year
|
| gptkbp:has_spectral_type |
gptkb:WC
WN WO |
| https://www.w3.org/2000/01/rdf-schema#label |
Wolf-Rayet stars
|
| gptkbp:is_associated_with |
Wolf-Rayet nebulae
|
| gptkbp:is_believed_to |
the end stage of some massive stars
the progenitors of long-duration gamma-ray bursts |
| gptkbp:is_common_in |
metal-rich environments
|
| gptkbp:is_essential_for |
understanding galaxy evolution
understanding stellar evolution |
| gptkbp:is_found_in |
star-forming regions
star clusters |
| gptkbp:is_located_in |
gptkb:the_Milky_Way
other galaxies |
| gptkbp:is_often_accompanied_by |
supernova explosions
|
| gptkbp:is_often_associated_with |
supernovae
|
| gptkbp:is_often_compared_to |
more than 20 solar masses
|
| gptkbp:is_often_seen_in |
regions of active star formation
|
| gptkbp:is_often_used_in |
stellar population studies
|
| gptkbp:is_recognized_by |
their unique spectra
|
| gptkbp:is_studied_in |
gptkb:Chandra_X-ray_Observatory
gptkb:Hubble_Space_Telescope astrophysics ground-based telescopes |
| gptkbp:lifespan |
a few million years
|
| gptkbp:scientific_classification |
their emission line strengths
|
| gptkbp:bfsParent |
gptkb:Carina_Nebula
|
| gptkbp:bfsLayer |
4
|