subgiant : Related Words Words similar in meaning to subgiant
- subgiant star«
- star«
- subgiant branch«
- main sequence«
- giant star«
- subgiants«
- luminosity«
- red giant branch«
- core«
- hydrogen«
- r diagram«
- temperature«
- mass«
- helium core mass«
- main sequence star«
- low metallicity star«
- metallicity«
- convective core«
- red giant«
- hydrogen shell«
- cluster«
- supergiant«
- term subgiant«
- schönberg–chandrasekhar mass«
- main sequence turnoff«
- evolutionary subgiants«
- core hydrogen exhaustion«
- balmer line profile«
- subgiant luminosity class«
- hydrogen shell fusion«
- sequence star«
- η cephei«
- schönberg–chandrasekhar limit«
- spectral luminosity class«
- lower mass star«
- shell«
- hertzsprung gap«
- outer layer«
- giant branch«
- low metallicity«
- delta scuti variable«
- sun«
- initial mass«
- spectral class«
- mass star«
- herculis«
- evolution«
- aldebaran«
- thermal equilibrium«
- start«
- fusion«
- hook«
- absolute magnitude«
- degenerate«
- transition«
- τ bootis«
- π scorpii«
- θ2 orionis a«
- θ bootis«
- η bootis«
- ζ serpentis«
- δ scorpii«
- δ circini system«
- α centauri b«
- unusual chemical peculiarity«
- typical log(g«
- true giant star«
- tio line strength«
- subsequent core helium fusion«
- subgiant class«
- stellar evolutionary track«
- star fk com«
- sr/fe line ratio«
- separate subgiant branch«
- r limit«
- pronounced subgiant branch«
- obvious giant star«
- massive subgiant star«
- massive subgiant evolution«
- massive o class main sequence star«
- massive helium core«
- many line ratio«
- luminosity indicator«
- low mass core«
- late b main sequence«
- kappa andromedae b.«
- k class star«
- iv star«
- it temperature increase«
- initial main sequence position«
- hydrogen shell increase«
- hot massive convective core«
- hook duration«
- fusion increase«
- fe line strength«
- f main sequence«
- evolutionary subgiant branch«
- entire star contract«
- entire convective region«
- diagonal main sequence band«
- coronal emission strength«
- core hydrogen fusion«
- cooler subgiants«
- cool main sequence star«
- ca h line profile«
- b main sequence«
- ω centauri«
- μ cancri«
- λ ursae majoris«
- λ scorpii«
- ζ cassiopeiae«
- γ orionis«
- β aquilae«
- yerkes luminosity class«
- surface effective temperature«
- subgiant spectral type«
- spectral type k3«
- population i«
- o class star«
- massive stars«
- luminosity relative«
- giant spectral luminosity class«
- extreme population ii«
- exact initial mass«
- core temperature increase«
- change visible«
- b main sequence star«
- absolute feature«
- stage«
- τ herculis«
- β scorpii«
- β aurigae«
- yerkes spectral classification system«
- sv vulpeculae«
- main sequence band«
- luminosity class iv«
- log(g«
- larger helium core«
- core hydrogen burning«
- core contraction«
- cno cycle fusion«
- ca h«
- blended spectrum«
- ι herculis«
- θ ophiuchi«
- β cephei«
- β ca«
- tio band«
- star cooler«
- dimensional classification scheme«
- θ draconis«
- mass stars«
- k hotter«
- giant luminosity class«
- class o star«
- μ herculis«
- γ cassiopeiae«
- cepheid instability strip«
- diagram«
- γ cephei«
- k star«
- hydrogen fuse«
- δ herculis«
- γ serpentis«
- strong temperature gradient«
- luminosity increase«
- h–r diagram«
- β serpentis«
- sequence lifetime«
- centre outwards«
- example«
- luminosity class v«
- external indication«
- degenerate helium core«
- core mass«
- classical cepheid variable«
- helium core«
- strong emission«
- envelop«
- o line«
- dimensional scheme«
- axis«
- wing width«
- typical lifetime«
- solar metallicity«
- lower metallicity«
- geminorum«
- chemical abundance«
- magnitude diagram«
- entire star«
- blue loop«
- broader wing«
- internal configuration«
- instability strip«
- beta cephei variable«
- similar spectrum«
- overshooting«
- line strength«
- standard star«
- later analysis«
- such star«
- crossing«
- variability«
- spectral feature«
- spectral classification«
- similar difference«
- k line«
- hertzsprung«
- larger fraction«
- class star«
- persei«
- planets«
- typical approach«
- andromedae«
- it mass«
- hertzsprung–russell diagram«
- class g«
- stellar population«
- scatter plot«
- key value«
- faint star«
- thick shell«
- luminosity class«
- procyon«
- surface gravity«
- pegasi«
- original star«
- primary star«
- value«
- current age«
- energy output«
- properties«
- outer envelope«
- centauri«
- spectral type«
- increase«
- massive star«
- relative strength«
- weight«
- expansion«
- double star«
- globular cluster«
- rate«
- strength«
- keenan«
- several type«
- central core«
- narrow range«
- energy«
- apparent lack«
- effective temperature«
- type star«
- white dwarf«
- variable star«
- standard«
- difference«
- class b«
- a5«
- com«
- roman numeral«
- age«
- initial stage«
- convection«
- lithium«
- a3«
- time«
- helium«
- fe«
- a2«
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