star formation regions in Milky Way

GPTKB entity

Statements (60)
Predicate Object
gptkbp:instance_of gptkb:astronomy
gptkbp:are_mapped_by space telescopes
gptkbp:are_often_found_near gptkb:supernova_remnants
gptkbp:are_often_identified_by their emission lines
gptkbp:are_often_obscured_by interstellar dust
gptkbp:are_often_studied_through computer simulations
gptkbp:are_part_of giant molecular clouds
gptkbp:can_be_found_in the Scutum-Centaurus Arm
the Perseus Arm
gptkbp:can_be_traced_using hydrogen emissions
gptkbp:can_collapse_under gravitational forces
gptkbp:can_lead_to star clusters
planetary systems
gptkbp:contains molecular clouds
gptkbp:emissions_standard gptkb:infrared_radiation
https://www.w3.org/2000/01/rdf-schema#label star formation regions in Milky Way
gptkbp:include gptkb:Orion_Nebula
gptkb:Eagle_Nebula
gptkb:Lagoon_Nebula
gptkbp:is_a_site_of stellar birth
gptkbp:is_affected_by cosmic rays
stellar feedback
gptkbp:is_associated_with young stellar objects
massive stars
gptkbp:is_characterized_by high temperatures
stellar nurseries
high density of gas and dust
gptkbp:is_essential_for understanding galaxy formation
galactic evolution
understanding cosmic evolution
stellar evolution studies
chemical enrichment
understanding star formation processes
gptkbp:is_found_in H II regions
gptkbp:is_influenced_by magnetic fields
stellar winds
supernova explosions
gptkbp:is_linked_to the lifecycle of stars
gptkbp:is_observed_in optical wavelengths
radio telescopes
radio wavelengths
gptkbp:is_often_associated_with gptkb:starburst_galaxies
dark nebulae
galactic outflows
star formation rates.
gptkbp:is_often_seen_in spiral arms
the Orion Arm
infrared surveys
gptkbp:is_rich_in young stars
heavy elements
gptkbp:is_studied_for their dynamics
gptkbp:is_studied_in gptkb:spectroscopy
gptkb:astronomy
astrophysics
galactic astronomy
gptkbp:is_targeted_at galactic collisions
gptkbp:located_in gptkb:Milky_Way_galaxy
gptkbp:trigger_type further star formation
gptkbp:bfsParent gptkb:Lagoon_Nebula
gptkbp:bfsLayer 6