|
gptkbp:instance_of
|
gptkb:Supernova
|
|
gptkbp:associated_with
|
gptkb:galaxy_NGC_4321
|
|
gptkbp:conducts_research_on
|
gptkb:interstellar_medium
cosmic rays
cosmic microwave background
|
|
gptkbp:contains
|
heavy elements
|
|
gptkbp:diameter
|
approximately 10 light-years
|
|
gptkbp:discovered_by
|
gptkb:Hubble_Space_Telescope
|
|
gptkbp:distance_from_earth
|
approximately 50 million light-years
|
|
gptkbp:emissions_standard
|
X-ray emission
|
|
gptkbp:exploded_in
|
gptkb:1994
|
|
gptkbp:has_historical_significance
|
first observed in 1994
|
|
gptkbp:has_remnant_structure
|
shell structure
|
|
gptkbp:has_spectral_type
|
Type II-P
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
SN 1994 I remnant
|
|
gptkbp:investigates
|
magnetic fields
chemical enrichment of the universe
shock wave dynamics
|
|
gptkbp:is_analyzed_in
|
chemical composition
energy output
radiation signatures
|
|
gptkbp:is_associated_with
|
gptkb:Supernova
supernova remnants in general
|
|
gptkbp:is_considered
|
galaxy formation theories
astrophysics studies
|
|
gptkbp:is_described_as
|
galactic dynamics
supernova mechanisms
|
|
gptkbp:is_documented_in
|
gptkb:literature
astronomical surveys
astronomical catalogs
|
|
gptkbp:is_examined_in
|
gamma-ray emissions
light echo phenomena
shock interaction
|
|
gptkbp:is_in
|
constellation Coma Berenices
|
|
gptkbp:is_noted_for
|
its brightness
its role in star formation.
its expansion rate
|
|
gptkbp:is_observed_in
|
gptkb:Chandra_X-ray_Observatory
radio wavelengths
infrared wavelengths
|
|
gptkbp:is_part_of
|
gptkb:Virgo_cluster
galactic evolution studies
high-energy astrophysics research
supernova remnant classification
stellar explosion studies
|
|
gptkbp:is_related_to
|
gptkb:supernova_1987_A
stellar nucleosynthesis
|
|
gptkbp:is_related_to_research_on
|
gptkb:dark_matter
|
|
gptkbp:is_studied_for
|
stellar evolution
elemental synthesis
stellar mass loss
neutrino emissions
|
|
gptkbp:is_studied_in
|
gptkb:astronomy
|
|
gptkbp:is_used_in
|
cosmology research
|
|
gptkbp:is_visible_from
|
gptkb:Earth
|
|
gptkbp:lighting
|
peculiar light curve
|
|
gptkbp:located_in
|
gptkb:Messier_100
|
|
gptkbp:notable_for
|
bright optical light
|
|
gptkbp:remnant_of
|
gptkb:Giant
|
|
gptkbp:type
|
gptkb:Type_II_supernova_remnant
|
|
gptkbp:bfsParent
|
gptkb:SN_1994_I
|
|
gptkbp:bfsLayer
|
5
|