Statements (50)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Nova
|
| gptkbp:affects |
surrounding interstellar medium
|
| gptkbp:are_part_of |
stellar evolution studies
stellar explosion classification the broader category of novae. |
| gptkbp:can_cause |
brightness increase
|
| gptkbp:can_detect |
space telescopes
|
| gptkbp:can_exhibit_variability_in |
outburst frequency
|
| gptkbp:can_involve |
gptkb:Dwarves
|
| gptkbp:can_lead_to |
nova remnant formation
|
| gptkbp:can_recur_every |
few years to decades
|
| gptkbp:characterized_by |
multiple outbursts
|
| gptkbp:example |
RS Ophiuchi
T Coronae Borealis U Scorpii |
| gptkbp:exhibits |
spectral lines
|
| https://www.w3.org/2000/01/rdf-schema#label |
Recurrent Novae
|
| gptkbp:impact |
galactic chemical evolution
|
| gptkbp:influence |
stellar population dynamics
|
| gptkbp:investigates |
their chemical composition
|
| gptkbp:is_associated_with |
accretion disks
mass transfer in binaries |
| gptkbp:is_considered |
important for cosmology
a subclass of novae |
| gptkbp:is_different_from |
classical novae
|
| gptkbp:is_essential_for |
understanding stellar processes
the study of binary systems |
| gptkbp:is_monitored_by |
astronomical observatories
|
| gptkbp:is_observed_in |
gptkb:the_Milky_Way
various wavelengths different galaxies different outburst mechanisms |
| gptkbp:is_recognized_by |
specific light patterns
|
| gptkbp:is_related_to |
gptkb:Type_Ia_supernovae
supernova progenitors |
| gptkbp:is_studied_in |
gptkb:spectroscopy
astrophysics computer simulations light curves |
| gptkbp:is_targeted_at |
massive companion stars
|
| gptkbp:is_tested_for |
stellar evolution theories
|
| gptkbp:key |
stellar lifecycle
|
| gptkbp:occurs_in |
binary star systems
|
| gptkbp:provides_information_on |
nuclear fusion processes
stellar mass transfer rates |
| gptkbp:release_energy_of |
10^37 to 10^38 joules
|
| gptkbp:scientific_classification |
thermonuclear explosions
|
| gptkbp:type |
Stellar explosion
|
| gptkbp:bfsParent |
gptkb:Cataclysmic_Variable
|
| gptkbp:bfsLayer |
5
|