Statements (101)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Supernova
|
| gptkbp:affects |
galactic chemical evolution
|
| gptkbp:are |
standard candles
thermonuclear explosions |
| gptkbp:are_a_key_factor_in_understanding |
the large-scale structure of the universe
|
| gptkbp:are_brighter_than |
most other types of supernovae
|
| gptkbp:are_classified_based_on |
their light curves
|
| gptkbp:are_detected_through |
their light emissions
|
| gptkbp:are_essential_for_measuring |
the scale of the universe
|
| gptkbp:are_important_for_determining |
the age of the universe
|
| gptkbp:are_important_for_measuring |
the expansion rate of the universe
|
| gptkbp:are_less_luminous_than |
gptkb:Type_II_supernovae
|
| gptkbp:are_often_used_to_test |
theories of gravity
|
| gptkbp:are_part_of |
gptkb:standard_model_of_cosmology
Hubble diagram stellar evolution process |
| gptkbp:are_part_of_the_research_into |
the evolution of the universe over time
|
| gptkbp:are_significant_for_their_role_in |
the synthesis of iron in the universe
|
| gptkbp:are_thought_to_occur_in |
binary star systems
|
| gptkbp:are_used_to_infer |
the expansion rate of the universe
|
| gptkbp:are_used_to_measure |
cosmic distances
|
| gptkbp:are_used_to_refine |
the value of the Hubble constant
|
| gptkbp:are_used_to_test |
the cosmological principle
|
| gptkbp:can_be_detected_up_to |
billions of light-years away
|
| gptkbp:can_be_used_to_calibrate |
other distance measurement methods
|
| gptkbp:can_be_used_to_infer |
the presence of dark energy
|
| gptkbp:can_detect |
the infrared spectrum
ground-based and space telescopes |
| gptkbp:can_lead_to |
the formation of neutron stars or black holes
|
| gptkbp:can_provide_evidence_for |
the existence of dark energy
|
| gptkbp:contribute_to_our_understanding_of |
gptkb:dark_matter
|
| gptkbp:contribution |
the chemical enrichment of the universe
|
| gptkbp:formed |
neutron stars or black holes
|
| gptkbp:has_a_focus_on |
astronomical surveys and missions.
current astronomical research. |
| gptkbp:have_a_characteristic_light_curve_shape_that |
is used for classification
|
| gptkbp:have_a_characteristic_light_curve_that |
rises quickly and then declines
|
| gptkbp:have_a_consistent_peak_brightness |
which allows for distance estimation
|
| gptkbp:have_a_light_curve_that |
follows a specific pattern
|
| gptkbp:have_a_peak_brightness_of |
approximately -19.3 magnitudes
|
| gptkbp:have_been_used_to_discover |
the accelerated expansion of the universe
|
| https://www.w3.org/2000/01/rdf-schema#label |
Type Ia supernovae
|
| gptkbp:is_a_key_component_of |
modern astrophysics
the cosmic distance ladder |
| gptkbp:is_a_source_of |
light in the universe during their peak brightness
|
| gptkbp:is_a_subject_of |
the field of high-energy astrophysics
|
| gptkbp:is_analyzed_in |
the Hubble constant
|
| gptkbp:is_associated_with |
the Chandrasekhar limit
the end of a white dwarf's life |
| gptkbp:is_characterized_by |
a lack of hydrogen lines in their spectra
|
| gptkbp:is_critical_for |
the fate of the universe
|
| gptkbp:is_essential_for |
gptkb:cosmology
stellar evolution the fate of the universe stellar nucleosynthesis galaxy formation and evolution |
| gptkbp:is_explored_in |
the physics of stellar explosions
|
| gptkbp:is_influenced_by |
the metallicity of the progenitor star
|
| gptkbp:is_involved_in |
chemical enrichment of the interstellar medium
|
| gptkbp:is_linked_to |
the end stages of stellar evolution in certain stars
|
| gptkbp:is_observed_in |
distant galaxies
various wavelengths of light various wavelengths including optical and infrared the local universe |
| gptkbp:is_often_associated_with |
gptkb:Type_Ia_supernova_remnants
|
| gptkbp:is_often_compared_to |
gptkb:Type_II_supernovae
|
| gptkbp:is_often_involved_in |
scientific papers and studies
|
| gptkbp:is_often_seen_in |
gptkb:elliptical_galaxies
star-forming regions |
| gptkbp:is_often_used_in |
other cosmological observations
|
| gptkbp:is_significant_for |
cosmological distance measurements
|
| gptkbp:is_studied_for |
galaxy formation and evolution
the physics of supernova explosions impact on galaxy dynamics |
| gptkbp:is_studied_in |
astrophysics and cosmology
spectroscopy and photometry the formation of heavy elements the mechanisms of supernova explosions various telescopes and observatories |
| gptkbp:is_targeted_at |
the accretion of matter from a companion star
mergers of white dwarfs the Chandrasekhar limit being exceeded |
| gptkbp:is_used_by |
standard candles in cosmology
|
| gptkbp:model |
hydrodynamic simulations
|
| gptkbp:named_after |
the type of progenitor system involved
|
| gptkbp:occurs_in |
binary star systems
old stellar populations |
| gptkbp:produces |
iron and other heavy elements
|
| gptkbp:provides_information_on |
the nature of dark matter
|
| gptkbp:research_focus |
observational cosmology
|
| gptkbp:result |
the accretion of matter onto a white dwarf
the thermonuclear explosion of a white dwarf |
| gptkbp:scientific_classification |
Type I supernovae
subtypes based on their light curves |
| gptkbp:typically_occur |
every few hundred years in a galaxy
|
| gptkbp:were_first_used_as_standard_candles_in |
the late 1990s
|
| gptkbp:bfsParent |
gptkb:White_Dwarf
gptkb:Supernova_1994_D gptkb:Supernova_Remnants gptkb:supernova_remnants |
| gptkbp:bfsLayer |
5
|