Statements (66)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Cloud_Computing_Service
|
| gptkbp:bfsLayer |
4
|
| gptkbp:bfsParent |
gptkb:Taurus-Auriga_molecular_cloud_complex
|
| gptkbp:associated_with |
gptkb:Taurus_constellation
|
| gptkbp:contains |
gptkb:Herschel_36
gptkb:Taurus-Auriga_star-forming_region star-forming regions dark nebulae star formation regions molecular hydrogen dark clouds dense cores starless cores star-forming clumps dense molecular filaments |
| gptkbp:depicted_in |
gptkb:physicist
northern hemisphere optical wavelengths southern hemisphere radio wavelengths infrared wavelengths Earth's surface submillimeter wavelengths |
| gptkbp:distance |
approximately 450 light-years
450 light years |
| https://www.w3.org/2000/01/rdf-schema#label |
Taurus Molecular Cloud
|
| gptkbp:is_associated_with |
gptkb:Taurus_constellation
gptkb:Taurus-Auriga_star-forming_region star formation regions |
| gptkbp:is_characterized_by |
cold temperatures
molecular gas high density of gas and dust molecular outflows high angular momentum high extinction high molecular density |
| gptkbp:is_home_to |
gptkb:automobile
young stellar objects star clusters massive stars pre-main-sequence stars young stellar clusters protostars |
| gptkbp:is_part_of |
gptkb:Taurus_Molecular_Cloud_complex
gptkb:interstellar_medium gptkb:star gptkb:Milky_Way_Galaxy star-forming regions star formation regions interstellar clouds Giant Molecular Clouds |
| gptkbp:is_rich_in |
gptkb:carbon_monoxide
|
| gptkbp:is_studied_in |
gptkb:observatory
chemical composition stellar evolution stellar nurseries star formation processes molecular cloud dynamics molecular cloud structure interstellar chemistry |
| gptkbp:length |
approximately 20 light years across
|
| gptkbp:located_in |
gptkb:Taurus_constellation
|
| gptkbp:mass |
about 1000 solar masses
|
| gptkbp:notable_products |
B213
L1495 L1517 |