Beta Cephei variable
Beta Cephei variables, also known as Beta Canis Majoris stars, are variable stars that exhibit small rapid variations in their brightness due to pulsations of the stars' surfaces, thought due to the unusual properties of iron at temperatures of 200,000 K in their interiors. These stars are usually hot blue-white stars of spectral class B and should not be confused with Cepheid variables, which are named after Delta Cephei and are luminous supergiant stars.
10 Lacertae12 Lacertae15 Canis Majoris16 Lacertae19 Monocerotis1 Camelopardalis1 Vulpeculae22 Orionis27 Canis Majoris2 Vulpeculae42 Camelopardalis53 Arietis53 Piscium68 HerculisAlpha LupiAlpha MuscaeAlpha PyxidisAstronomical objectBW VulpeculaeBeta Canis MajorisBeta Canis Majoris starBeta CentauriBeta CepheiBeta Cephei starBeta Cephei variablesBeta Cepheid starBeta LupiBeta cephei variableCanis MajorChi CarinaeChi CentauriCoRoTCollinder 135Delta CetiDelta LupiEdwin Brant FrostEpsilon CentauriEpsilon LupiEpsilon PerseiEta Hydrae
Link from a Wikipage to another Wikipage
10 Lacertae12 Lacertae15 Canis Majoris16 Lacertae19 Monocerotis27 Canis Majoris2 Vulpeculae53 Arietis53 PisciumAlpha LupiAlpha MuscaeAlpha PyxidisBW VulpeculaeBeta Canis MajorisBeta CentauriBeta CepheiBeta LupiChi CentauriDelta CetiDelta LupiEpsilon CentauriEpsilon PerseiGamma PegasiImai (star)Iota Canis MajorisIota HerculisJ CentauriKappa ScorpiiLambda CrucisLambda ScorpiiMerope (star)NW PuppisNu CentauriOmega1 CygniOmega1 ScorpiiPT PuppisPi2 CygniSigma CassiopeiaeSpicaTau1 Lupi
variable
primaryTopic
Beta Cephei variable
Beta Cephei variables, also known as Beta Canis Majoris stars, are variable stars that exhibit small rapid variations in their brightness due to pulsations of the stars' surfaces, thought due to the unusual properties of iron at temperatures of 200,000 K in their interiors. These stars are usually hot blue-white stars of spectral class B and should not be confused with Cepheid variables, which are named after Delta Cephei and are luminous supergiant stars.
has abstract
Beta Cephei izar aldakorrak iz ...... izarragatik deituak bait dira.
@eu
Beta Cephei variables, also kn ...... are luminous supergiant stars.
@en
Beta Cephei-veranderlijken (BC ...... rnoemd zijn naar Delta Cephei.
@nl
Els estels variables Beta Ceph ...... menades així per Delta Cephei.
@ca
Gwiazdy typu Beta Cephei – gwi ...... miennych typu Beta Cephei są .
@pl
Hvězdy typu Beta Cephei, také ...... dy hvězdami typu delta Cephei.
@cs
Las estrellas variables Beta C ...... llamadas así por Delta Cephei.
@es
Les (étoiles) variables de typ ...... nommées d'après Delta Cephei.
@fr
Una variabile Beta Cephei, chi ...... della superficie della stella.
@it
Variáveis Beta Cephei são estr ...... adas a partir de Delta Cephei.
@pt
Wikipage page ID
page length (characters) of wiki page
Wikipage revision ID
1,021,383,171
Link from a Wikipage to another Wikipage
wikiPageUsesTemplate
subject
hypernym
type
comment
Beta Cephei izar aldakorrak iz ...... izarragatik deituak bait dira.
@eu
Beta Cephei variables, also kn ...... are luminous supergiant stars.
@en
Beta Cephei-veranderlijken (BC ...... rnoemd zijn naar Delta Cephei.
@nl
Els estels variables Beta Ceph ...... amb un període de 4,57 hores.
@ca
Gwiazdy typu Beta Cephei – gwi ...... mi podolbrzymami i olbrzymami.
@pl
Hvězdy typu Beta Cephei, také ...... dy hvězdami typu delta Cephei.
@cs
Las estrellas variables Beta C ...... con un período de 4,57 horas.
@es
Les (étoiles) variables de typ ...... ur une période de 4,57 heures.
@fr
Una variabile Beta Cephei, chi ...... della superficie della stella.
@it
Variáveis Beta Cephei são estr ...... tem um período de 4,57 horas.
@pt
label
Beta Cephei izar aldakor
@eu
Beta Cephei variable
@en
Beta Cephei-variabel
@sv
Beta Cephei-veranderlijken
@nl
Beta-Cephei-Stern
@de
Estrella variable Beta Cephei
@es
Gwiazdy zmienne typu Beta Cephei
@pl
Hvězda typu Beta Cephei
@cs
Variabile Beta Cephei
@it
Variable Beta Cephei
@ca