Taurus-Auriga molecular cloud complex
GPTKB entity
Statements (64)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Cloud_Computing_Service
|
| gptkbp:associated_with |
star formation
|
| gptkbp:average_temperature |
10-20 K
|
| gptkbp:contains |
gptkb:Taurus_Molecular_Cloud
gptkb:L1521_F L1495 dark clouds dense cores L1517 L1536 L1544 |
| gptkbp:depicted_in |
gptkb:physicist
|
| gptkbp:distance |
approximately 450 light years
|
| gptkbp:has_influence_on |
stellar evolution
|
| https://www.w3.org/2000/01/rdf-schema#label |
Taurus-Auriga molecular cloud complex
|
| gptkbp:is_associated_with |
gptkb:Auriga_constellation
gptkb:Taurus_constellation |
| gptkbp:is_characterized_by |
X-ray emissions
chemical reactions spectral lines infrared emissions star-forming regions dark nebulae low temperature molecular gas dynamics chemical enrichment star cluster formation chemical abundances radio emissions turbulence effects molecular line emissions high density regions optical emissions stellar feedback effects chemical complexity magnetic field influence dust presence gas presence gravitational collapse phenomena interstellar dust composition molecular cloud fragmentation molecular cloud lifecycle molecular clouds interactions molecular hydrogen presence stellar population diversity |
| gptkbp:is_home_to |
young stellar objects
protostars pre-main sequence stars |
| gptkbp:is_observed_in |
gptkb:Subaru_Telescope
gptkb:Hubble_Space_Telescope gptkb:James_Clerk_Maxwell_Telescope |
| gptkbp:is_part_of |
gptkb:Orion_Arm
gptkb:Milky_Way_galaxy |
| gptkbp:is_studied_in |
gptkb:interstellar_medium
astrophysics star formation processes molecular cloud dynamics |
| gptkbp:length |
about 20 parsecs
|
| gptkbp:located_in |
gptkb:Taurus_constellation
|
| gptkbp:mass |
about 1000 solar masses
|
| gptkbp:part_of |
Giant Molecular Clouds
|
| gptkbp:significance |
star formation research
|
| gptkbp:bfsParent |
gptkb:automobile
|
| gptkbp:bfsLayer |
3
|