Stellar physics. Unified Astronomy Thesaurus

Stellar physics

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NT1 ↓ Black hole physics ►▼
- NT2 ↓ Bekenstein–Hawking entropy
- NT2 ↓ Black hole spin-flip
- NT2 ↓ Black hole thermodynamics
- NT2 ↓ Ergosphere
- NT2 ↓ Hawking radiation
- NT2 ↓ Kruskal diagram
- NT2 ↓ Penrose process
- NT2 ↓ Photon sphere
- NT2 ↓ Quasinormal modes
- NT2 ↓ Trans-Planckian physics
NT1 ↓ Blazhko effect
NT1 ↓ Interstellar dynamics
NT1 ↓ Radiation variability ►▼
- NT2 ↓ High radiation state
- NT2 ↓ Low radiation state
- NT2 ↓ Superhumps
NT1 ↓ Solar physics ►▼
- NT2 ↓ CNO anomaly
- NT2 ↓ Helioseismology ►▼
  - NT3 ↓ Helioseismic pulsations
  - NT3 ↓ Solar cycle ►▼
    - NT4 ↓ Active sun
    - NT4 ↓ Quiet sun
    - NT4 ↓ Sunspot cycle
  - NT3 ↓ Solar magnetic fields ►▼
    - NT4 ↓ Solar magnetic reconnection
- NT2 ↓ Solar abundances
- NT2 ↓ Solar activity ►▼
  - NT3 ↓ Solar activity cycles ►▼
    - NT4 ↓ Solar cycle variations
  - NT3 ↓ Solar flares ►▼
    - NT4 ↓ Radio flares
    - NT4 ↓ X-ray flares
  - NT3 ↓ Solar prominences ►▼
    - NT4 ↓ Quiescent prominence
  - NT3 ↓ Solar storm
  - NT3 ↓ Sun spots
  - NT3 ↓ Wilson effect
- NT2 ↓ Solar atmosphere ►▼
  - NT3 ↓ Chromosphere ►▼
    - NT4 ↓ Plages
  - NT3 ↓ Solar chromosphere
  - NT3 ↓ Solar corona ►▼
    - NT4 ↓ M region
    - NT4 ↓ Solar coronal holes
    - NT4 ↓ Solar coronal loops
    - NT4 ↓ Solar coronal streamers
  - NT3 ↓ Solar photosphere
  - NT3 ↓ Solar transition region
- NT2 ↓ Solar electromagnetic emission ►▼
  - NT3 ↓ Solar gamma ray emission
  - NT3 ↓ Solar radio emission
  - NT3 ↓ Solar ultraviolet emission
  - NT3 ↓ Solar X-ray emission
  - NT3 ↓ Visible solar emission
- NT2 ↓ Solar faculae
- NT2 ↓ Solar filaments
- NT2 ↓ Solar flares ►▼
  - NT3 ↓ Radio flares
  - NT3 ↓ X-ray flares
- NT2 ↓ Solar granulation ►▼
  - NT3 ↓ Supergranulation
- NT2 ↓ Solar interior ►▼
  - NT3 ↓ Solar core
- NT2 ↓ Solar magnetism
- NT2 ↓ Solar motion ►▼
  - NT3 ↓ Antapex
  - NT3 ↓ Apex
  - NT3 ↓ Solar atmospheric motions
- NT2 ↓ Solar oscillations
- NT2 ↓ Solar particle emission ►▼
  - NT3 ↓ Solar energetic particles
  - NT3 ↓ Solar neutrons
- NT2 ↓ Solar properties ►▼
  - NT3 ↓ Solar composition
  - NT3 ↓ Solar diameter
  - NT3 ↓ Solar irradiance
  - NT3 ↓ Solar magnetic fields ►▼
    - NT4 ↓ Solar magnetic reconnection
  - NT3 ↓ Solar magnetism
  - NT3 ↓ Solar mass
  - NT3 ↓ Solar rotation
- NT2 ↓ Solar radiation ►▼
  - NT3 ↓ Diffuse radiation
- NT2 ↓ Solar rotation
- NT2 ↓ Solar spicules ►▼
  - NT3 ↓ Fibrils
  - NT3 ↓ Mottles
  - NT3 ↓ Solar macrospicules
- NT2 ↓ Solar surface
- NT2 ↓ Solar transition region
- NT2 ↓ Solar wind ►▼
  - NT3 ↓ Heliopause
- NT2 ↓ Sunspots ►▼
  - NT3 ↓ Ephemeral active regions
  - NT3 ↓ Maunder minimum
  - NT3 ↓ Penumbral filaments
  - NT3 ↓ Sunspot groups ►▼
    - NT4 ↓ Bipolar sunspot groups
  - NT3 ↓ Sunspot number
NT1 ↓ Star formation
NT1 ↓ Starspots ►▼
- NT2 ↓ Sunspots ►▼
  - NT3 ↓ Ephemeral active regions
  - NT3 ↓ Maunder minimum
  - NT3 ↓ Penumbral filaments
  - NT3 ↓ Sunspot groups ►▼
    - NT4 ↓ Bipolar sunspot groups
  - NT3 ↓ Sunspot number
NT1 ↓ Stellar dynamics ►▼
- NT2 ↓ Supernova dynamics
NT1 ↓ Stellar evolution ►▼
- NT2 ↓ Asymptotic giant branch
- NT2 ↓ Carbon flash
- NT2 ↓ Dredge-up
- NT2 ↓ Early stellar evolution
- NT2 ↓ Funneling
- NT2 ↓ Harman-Seaton sequence
- NT2 ↓ Helium flashes ►▼
  - NT3 ↓ Helium shell flashes
- NT2 ↓ Helmholtz-Kelvin contraction
- NT2 ↓ Hess diagram
- NT2 ↓ Initial mass function
- NT2 ↓ Kelvin–Helmholtz timescale
- NT2 ↓ Late stellar evolution
- NT2 ↓ Solar evolution ►▼
  - NT3 ↓ Solar nebulae
- NT2 ↓ Star formation
- NT2 ↓ Stellar evolutionary tracks ►▼
  - NT3 ↓ Hayashi track
  - NT3 ↓ Henyey track
- NT2 ↓ Stellar progenitors ►▼
  - NT3 ↓ Nova progenitors
  - NT3 ↓ Supernova progenitors
- NT2 ↓ Supernova evolution
NT1 ↓ Stellar kinematics ►▼
- NT2 ↓ Stellar motion ►▼
  - NT3 ↓ Proper motions
  - NT3 ↓ Solar motion ►▼
    - NT4 ↓ Antapex
    - NT4 ↓ Apex
    - NT4 ↓ Solar atmospheric motions
- NT2 ↓ Stellar rotation ►▼
  - NT3 ↓ Gravity darkening
  - NT3 ↓ Radiative braking
NT1 ↓ Stellar phenomena ►▼
- NT2 ↓ Burst astrophysics ►▼
  - NT3 ↓ Gamma-ray bursts
  - NT3 ↓ Optical bursts
  - NT3 ↓ Radio bursts
  - NT3 ↓ Rapid bursts
  - NT3 ↓ X-ray bursts
- NT2 ↓ Coronal mass ejections
- NT2 ↓ Heliosphere interstellar medium interactions
- NT2 ↓ Stellar flares ►▼
  - NT3 ↓ Disk flaring
  - NT3 ↓ Optical flares
- NT2 ↓ Stellar mass loss ►▼
  - NT3 ↓ Plasma jets
- NT2 ↓ Stellar pulsations ►▼
  - NT3 ↓ Multi-periodic pulsation ►▼
    - NT4 ↓ Double-mode pulsation
  - NT3 ↓ Non-radial pulsations
  - NT3 ↓ Pulsation modes
  - NT3 ↓ Radial pulsations
NT1 ↓ Stellar properties ►▼
- NT2 ↓ Expanding stellar envelopes
- NT2 ↓ Starlight polarization
- NT2 ↓ Stellar accretion
- NT2 ↓ Stellar activity
- NT2 ↓ Stellar ages
- NT2 ↓ Stellar colors
- NT2 ↓ Stellar effective temperatures
- NT2 ↓ Stellar luminosities
- NT2 ↓ Stellar magnetic fields
- NT2 ↓ Stellar magnitudes
- NT2 ↓ Stellar mass functions
- NT2 ↓ Stellar masses
- NT2 ↓ Stellar oscillations ►▼
  - NT3 ↓ Rapid stellar oscillations
  - NT3 ↓ Solar oscillations
- NT2 ↓ Stellar radii
- NT2 ↓ Stellar spectral lines
- NT2 ↓ Stellar stability
- NT2 ↓ Stellar winds ►▼
  - NT3 ↓ Solar wind ►▼
    - NT4 ↓ Heliopause
NT1 ↓ Stellar structure ►▼
- NT2 ↓ Circumstellar shell ►▼
  - NT3 ↓ Dust shell
  - NT3 ↓ Rotating shell
  - NT3 ↓ Shell burning
- NT2 ↓ Convective envelope ►▼
  - NT3 ↓ Convective shells
- NT2 ↓ Convective zone
- NT2 ↓ Polytropes
- NT2 ↓ Stellar atmospheres ►▼
  - NT3 ↓ Chromosphere ►▼
    - NT4 ↓ Plages
  - NT3 ↓ Chromospheres
  - NT3 ↓ Coronae ►▼
    - NT4 ↓ Coronal dimming
    - NT4 ↓ Coronal hole
    - NT4 ↓ Coronal lines
    - NT4 ↓ Coronal loops
    - NT4 ↓ Coronal plumes
    - NT4 ↓ Coronal transients
    - NT4 ↓ E corona
    - NT4 ↓ F corona
    - NT4 ↓ K corona
    - NT4 ↓ Solar corona ►
  - NT3 ↓ Photosphere ►▼
    - NT4 ↓ Granule
    - NT4 ↓ Stellar faculae
  - NT3 ↓ Photospheres
  - NT3 ↓ Solar atmosphere ►▼
    - NT4 ↓ Chromosphere ►
    - NT4 ↓ Solar chromosphere
    - NT4 ↓ Solar corona ►
    - NT4 ↓ Solar photosphere
    - NT4 ↓ Solar transition region
  - NT3 ↓ Solar photosphere
- NT2 ↓ Stellar composition ►▼
  - NT3 ↓ Stellar chemical composition
  - NT3 ↓ Stellar elemental abundances
- NT2 ↓ Stellar gas distribution
- NT2 ↓ Stellar interior ►▼
  - NT3 ↓ Stellar cores ►▼
    - NT4 ↓ Stellar inner core
- NT2 ↓ Stellar surfaces
- NT2 ↓ Strömgren spheres

Related terms

RT⇆ Gravitation
RT⇆ Hertzsprung Russell diagrams

Date of creation

18-Dec-2013

Accepted term

18-Dec-2013

Descendant terms

195

ARK

ark:/99152/t331z0okrxlmo4

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Stellar physics

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