Herbig– Haro objects

GPTKB entity

Statements (54)
Predicate Object
gptkbp:instance_of gptkb:astronomy
gptkbp:are_key_indicators_of massive star formation
gptkbp:are_often_associated_with_regions_of active star formation
gptkbp:are_often_imaged_in H-alpha light
gptkbp:are_part_of star-forming regions
gptkbp:are_typically_located_in molecular clouds
gptkbp:associated_with star formation
gptkbp:can ongoing star formation
gptkbp:can_be_found_in gptkb:the_Milky_Way
star-forming galaxies
gptkbp:can_be_found_in_regions_of high stellar density
gptkbp:can_be_used_to_trace stellar winds
gptkbp:can_detect space telescopes
gptkbp:can_exhibit_different morphologies
gptkbp:can_exhibit_variability_in brightness
gptkbp:can_indicate_presence_of molecular gas
gptkbp:characterized_by jets of gas
gptkbp:conducts_research_on cosmic evolution
gptkbp:discovered_by gptkb:George_Herbig
Guenther Haro
gptkbp:exhibits shock waves
spectral lines
https://www.w3.org/2000/01/rdf-schema#label Herbig– Haro objects
gptkbp:is_a_key_component_of star formation theory
gptkbp:is_analyzed_in chemical composition
magnetic fields
kinematics
the context of galactic evolution
gptkbp:is_associated_with outflows from young stars
gptkbp:is_essential_for understanding stellar evolution
gptkbp:is_explored_in the lifecycle of stars
gptkbp:is_found_in various galaxies
nebulae
gptkbp:is_observed_in infrared wavelengths
optical telescopes
gptkbp:is_often_associated_with molecular outflows
shock-excited emission
gptkbp:is_often_seen_in young stars
star clusters
gptkbp:is_recognized_as 1960s
gptkbp:is_related_to gptkb:Taurus
gptkbp:is_studied_in gptkb:interstellar_medium
astrophysics
radio telescopes
energy transfer processes
stellar feedback
gptkbp:is_visible_from optical wavelengths
gptkbp:named_after gptkb:George_Herbig
Guenther Haro
gptkbp:provides_information_on planetary formation
gptkbp:research_importance galactic dynamics
gptkbp:scientific_classification emission nebulae
gptkbp:bfsParent gptkb:George_Herbig
gptkbp:bfsLayer 7