|
gptkbp:instance_of
|
gptkb:Cloud_Computing_Service
|
|
gptkbp:bfsLayer
|
5
|
|
gptkbp:bfsParent
|
gptkb:Taurus_Molecular_Cloud
|
|
gptkbp:associated_with
|
star formation
|
|
gptkbp:contains
|
gptkb:TMC-1
gptkb:Taurus-Auriga_star-forming_region
gptkb:L1551
B213
L1495
L1527
B18
L1517
L1536
L1544
L1550
|
|
gptkbp:depicted_in
|
optical wavelengths
radio wavelengths
infrared wavelengths
|
|
gptkbp:distance
|
approximately 140 light-years from Earth
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Taurus Molecular Cloud complex
|
|
gptkbp:is_associated_with
|
gptkb:Taurus_star-forming_region
|
|
gptkbp:is_characterized_by
|
dense gas and dust
|
|
gptkbp:is_home_to
|
gptkb:Taurus_Molecular_Cloud
gptkb:TMC-1
gptkb:L1551
young stellar objects
B213
L1495
L1527
B18
L1517
L1536
L1544
L1550
|
|
gptkbp:is_located_near
|
gptkb:Perseus_Molecular_Cloud
gptkb:Orion_Molecular_Cloud
|
|
gptkbp:is_part_of
|
gptkb:Taurus_constellation
Giant Molecular Cloud
|
|
gptkbp:is_studied_in
|
astrophysics
chemical composition
stellar evolution
star formation processes
molecular cloud dynamics
|
|
gptkbp:length
|
approximately 20 parsecs across
|
|
gptkbp:located_in
|
gptkb:Taurus_constellation
|
|
gptkbp:mass
|
approximately 1000 solar masses
|