The rim of RCW 86

Image of part of a stellar remnant whose explosion was recorded in 185 AD. By studying this remnant in detail, a team of astronomers was able to solve the mystery of the Milky Way’s super-efficient particle accelerators. The team shows that the shock wave visible in this area is very efficient at accelerating particles and the energy used in this process matches the number of cosmic rays observed on Earth. North is toward the top right and east to the top left. The image is about 6 arc minutes across.

Créditos:

ESO/E. Helder & NASA/Chandra

Sobre a imagem

Id:eso0923a
Tipo:Observação
Data de divulgação:25 de Junho de 2009
Notícias relacionadas:eso0923
Tamanho:1672 x 947 px

Sobre o objeto

Nome:RCW 86
Tipo:Milky Way : Nebula : Type : Supernova Remnant
Distância:8000 anos-luz
Constellation:Circinus
Categoria:Nebulae

Formatos de imagens

JPEG grande
487,1 KB

Papéis de parede

1024x768
290,2 KB
1280x1024
381,0 KB
1600x1200
500,3 KB
1920x1200
599,7 KB
2048x1536
691,5 KB

Coordenadas

Position (RA):14 45 8.13
Position (Dec):-62° 17' 57.26"
Field of view:7.04 x 3.99 arcminutes
Orientação:O norte está a 70.6° à direita da vertical

Cores e filtros

BandaTelescópio
Raios XChandra X-ray Observatory
ÓpticoVery Large Telescope