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gptkbp:instance_of
|
gptkb:observatory
gptkb:organization
|
|
gptkbp:bfsLayer
|
7
|
|
gptkbp:bfsParent
|
gptkb:Gould_Belt
|
|
gptkbp:age
|
approximately 10 million years
approximately 16 million years
|
|
gptkbp:associated_with
|
star formation
|
|
gptkbp:contains
|
gptkb:Lower_Centaurus_Crux
gptkb:Upper_Centaurus_Lupus
gptkb:Upper_Scorpius
multiple star clusters
Sco O B2
|
|
gptkbp:depicted_in
|
gptkb:physicist
|
|
gptkbp:discovered_by
|
gptkb:20th_century
|
|
gptkbp:distance
|
approximately 100 parsecs
|
|
gptkbp:has_member
|
young stars
red giants
massive stars
blue supergiants
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Sco-Cen association
|
|
gptkbp:includes
|
Sco O B2
Cen O B1
Cen O B2
|
|
gptkbp:is_associated_with
|
gptkb:interstellar_medium
star formation
|
|
gptkbp:is_home_to
|
multiple stellar nurseries
|
|
gptkbp:is_known_for
|
high stellar density
|
|
gptkbp:is_located_near
|
the Galactic plane
|
|
gptkbp:is_part_of
|
gptkb:Centaurus_constellation
gptkb:Scorpius_constellation
gptkb:observatory
|
|
gptkbp:is_studied_in
|
astrophysics
stellar evolution
|
|
gptkbp:located_in
|
gptkb:Milky_Way
|
|
gptkbp:notable_person
|
gptkb:Gamma_Velorum
gptkb:Delta_Scorpii
gptkb:Fomalhaut
gptkb:Epsilon_Scorpii
gptkb:Sirius
gptkb:Zeta_Centauri
gptkb:Antares
gptkb:Aldebaran
gptkb:Vega
gptkb:Rho_Ophiuchi
gptkb:Achernar
gptkb:Procyon
Beta Scorpii
|
|
gptkbp:type
|
young stellar population
|