Statements (92)
Predicate | Object |
---|---|
gptkbp:instance_of |
gptkb:Atom
|
gptkbp:associated_with |
gptkb:LBN_762
gptkb:IC_348 gptkb:NGC_1333 |
gptkbp:average_temperature |
10-20 K
around 10-20 K |
gptkbp:contains |
gptkb:carbon_monoxide
star-forming regions dark nebulae young stellar objects molecular hydrogen dark clouds dense cores |
gptkbp:distance_from_earth |
approximately 600 light-years
600 light years |
https://www.w3.org/2000/01/rdf-schema#label |
Perseus molecular cloud
|
gptkbp:is_associated_with |
gptkb:Perseus_OB1_association
gptkb:Herbig-Haro_objects gptkb:Bok_globules stellar nurseries star formation activity |
gptkbp:is_home_to |
gptkb:Herbig-Haro_objects
gptkb:brown_dwarfs H II regions molecular gas star formation regions star clusters stellar nurseries bipolar outflows massive stars accretion disks dense cores massive star formation regions dust lanes molecular filaments pre-main-sequence stars stellar jets stellar associations molecular outflows circumstellar disks low-mass stars protostars high-density regions starless cores star-forming clumps dense molecular filaments chemical rich environments low-density regions pre-main sequence stars |
gptkbp:is_located_near |
gptkb:California_Nebula
gptkb:Taurus_molecular_cloud gptkb:Pleiades_star_cluster |
gptkbp:is_observed_in |
gptkb:Spitzer_Space_Telescope
gptkb:Hubble_Space_Telescope infrared telescopes radio telescopes |
gptkbp:is_part_of |
gptkb:Gould_Belt
gptkb:star gptkb:Milky_Way_galaxy star forming complex Perseus region |
gptkbp:is_rich_in |
interstellar dust
|
gptkbp:is_studied_for |
gptkb:interstellar_medium
gptkb:star chemical composition stellar evolution star formation rates molecular gas dynamics star cluster formation molecular cloud dynamics molecular line emissions molecular cloud structure interstellar chemistry interstellar medium properties |
gptkbp:is_studied_in |
astrophysics
star formation research |
gptkbp:is_visible_from |
gptkb:Earth
optical wavelengths radio wavelengths infrared wavelengths |
gptkbp:length |
approximately 20 parsecs
approximately 20 light years across |
gptkbp:located_in |
gptkb:Perseus_constellation
|
gptkbp:mass |
approximately 1000 solar masses
about 2000 solar masses |
gptkbp:part_of |
gptkb:Milky_Way_galaxy
Perseus molecular complex |
gptkbp:bfsParent |
gptkb:California_Nebula
gptkb:IC_348 gptkb:Mirfak gptkb:NGC_1333 |
gptkbp:bfsLayer |
6
|