Galáxia Anã de Canes Venatici I Ligações externas | Referências | Menu de navegaçãoThe Universe within 500000 light-years The Satellite GalaxiesTwo New Galaxies Orbiting the Milky WayStrange satellite galaxies revealed around Milky WayNew Milky Way companions found: SDSS-II first to view two dim dwarf galaxiesAstronomers Find Two New Milky Way Companions«A New Milky Way Dwarf Satellite in Canes Venatici»10.1086/505216«NASA/IPAC Extragalactic Database»eexpandindo-o

Galáxias anãs esferoidaisSubgrupo Via LácteaGrupo LocalConstelação de Canes Venatici


galáxias satélitesVia Láctea2006Leo ILeo IIgaláxia anã esferoidalconstelaçãoCanes Venaticianos-luz


























































































































































































































































































































































































































































































































































































































































































































































































































































































































Galáxia Anã de Canes Venatici

Dados observacionais (J2000)

Constelação

Canes Venatici
Tipo
dSph[1]

Asc. reta
13h 28m 03.5s[2]

Declinação
+33° 33′ 21″[2]
Distância
720 kal (220 kpc) [1]

Magnit. apar.
13.9[1][2]
Dimensões
31′ × 17′.0[1]

Outras denominações
CVn dSph[2]

Mapa

Canes Venatici constellation map.png

A Galáxia Anã de Canes Venatici I (CVN dSph) é um das mais distantes galáxias satélites da Via Láctea, a partir de 2006, juntamente com Leo I e Leo II.[1] É uma galáxia anã esferoidal na constelação de Canes Venatici, situada cerca de 720.000 anos-luz de distância. A galáxia tem aproximadamente 6,5 kly (2 kpc)[1] de diâmetro ao longo do eixo maior e é muito fraca. Consiste principalmente de uma população velha de estrelas pobres em metais.[1]



Ligações externas |



  • The Universe within 500000 light-years The Satellite Galaxies (Atlas of the Universe)


  • Two New Galaxies Orbiting the Milky Way (Ken Croswell) 19 de Abril, 2006


  • Strange satellite galaxies revealed around Milky Way Kimm Groshong (New Scientist) 17:00 24 de Abril 2006


  • New Milky Way companions found: SDSS-II first to view two dim dwarf galaxies (SDSS) 8 de Maio 2006


  • Astronomers Find Two New Milky Way Companions (SpaceDaily) 10 de Maio 2006


Referências |




  1. ↑ abcdefg Zucker, D. B.; et al. (2006). «A New Milky Way Dwarf Satellite in Canes Venatici». The Astrophysical Journal. 643 (2): L103–L106. doi:10.1086/505216  !CS1 manut: Uso explícito de et al. (link)


  2. ↑ abcd «NASA/IPAC Extragalactic Database». Results for CVn dSph. Consultado em 26 de novembro de 2006 
















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