Taurus-Auriga star-forming region
GPTKB entity
Statements (63)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:star
|
gptkbp:bfsLayer |
5
|
gptkbp:bfsParent |
gptkb:Taurus_Molecular_Cloud
|
gptkbp:associated_with |
star formation
|
gptkbp:contains |
gptkb:Taurus_Molecular_Cloud
gptkb:Barnard_68 gptkb:L1521_F L1495 L1517 |
gptkbp:depicted_in |
gptkb:physicist
optical wavelengths radio wavelengths infrared wavelengths |
gptkbp:distance |
approximately 450 light-years
|
gptkbp:features |
dark nebulae
young stellar objects |
https://www.w3.org/2000/01/rdf-schema#label |
Taurus-Auriga star-forming region
|
gptkbp:is_associated_with |
cosmic rays
star clusters star formation activity star formation history stellar feedback |
gptkbp:is_characterized_by |
molecular clouds
gravitational collapse molecular gas stellar winds molecular hydrogen active star formation dust lanes high density of gas star clusters formation chemical complexity high density of dust |
gptkbp:is_home_to |
gptkb:automobile
gptkb:brown_dwarfs stellar populations stellar nurseries massive stars emission nebulae young stellar clusters stellar associations protostars Herbig Ae/ Be stars star-forming cores |
gptkbp:is_part_of |
gptkb:interstellar_medium
gptkb:Gould_Belt gptkb:star gptkb:Milky_Way_galaxy star-forming complex local spiral arm star-forming environment |
gptkbp:is_studied_in |
gptkb:interstellar_medium
gptkb:observatory gptkb:star stellar evolution star formation rates chemical enrichment stellar kinematics molecular cloud dynamics stellar birth processes stellar mass distribution molecular cloud structure |
gptkbp:located_in |
gptkb:Taurus_constellation
|