Properties (48)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
star
|
| gptkbp:canLeadTo |
supernova in some cases
|
| gptkbp:characterizedBy |
high luminosity
large radius |
| gptkbp:hasAwards |
0.6 to 10 solar masses
|
| gptkbp:hasTechnology |
3000 to 5000 K
|
| https://www.w3.org/2000/01/rdf-schema#label |
Asymptotic Giant Branch
|
| gptkbp:involves |
helium burning
hydrogen burning |
| gptkbp:isAssociatedWith |
gptkb:red_giants
mass loss carbon stars dust formation |
| gptkbp:isAttendedBy |
environmental factors
mass transfer in binary systems |
| gptkbp:isChallengedBy |
planetary nebula phase
|
| gptkbp:isCharacterizedBy |
high mass loss rates
pulsations instabilities thermal pulses variable luminosity |
| gptkbp:isCitedBy |
main sequence phase
|
| gptkbp:isImportantFor |
galactic evolution
nucleosynthesis understanding stellar populations |
| gptkbp:isInfluencedBy |
stellar winds
stellar rotation |
| gptkbp:isLinkedTo |
nuclear fusion processes
chemical enrichment stellar metallicity |
| gptkbp:isPartOf |
gptkb:Hertzsprung-Russell_diagram
cosmic chemical evolution stellar lifecycle stellar evolution theory |
| gptkbp:isRelatedTo |
AGB stars
evolutionary tracks post-AGB stars |
| gptkbp:isServedBy |
star clusters
various galaxies near-infrared surveys |
| gptkbp:isStudiedIn |
spectroscopy
theoretical models stellar astrophysics stellar population synthesis |
| gptkbp:leads |
white dwarf formation
|
| gptkbp:occursIn |
low to intermediate mass stars
late stages of stellar evolution |
| gptkbp:produces |
planetary nebulae
|