The brilliant star VFTS 682 in the Large Magellanic Cloud
This view shows part of the very active star-forming region around the Tarantula Nebula in the Large Magellanic Cloud, a small neighbour of the Milky Way. At the exact centre lies the brilliant but isolated star VFTS 682 and to its lower right the very rich star cluster R 136. The origins of VFTS 682 are unclear — was it ejected from R 136 or did it form on its own? The star appears yellow-red in this view, which includes both visible-light and infrared images from the Wide Field Imager at the 2.2-metre MPG/ESO telescope at La Silla and the 4.1-metre infrared VISTA telescope at Paranal, because of the effects of dust.
Créditos:ESO/M.-R. Cioni/VISTA Magellanic Cloud survey. Acknowledgment: Cambridge Astronomical Survey Unit
Sobre a imagem
Id: | eso1117a |
Tipo: | Observação |
Data de divulgação: | 25 de Maio de 2011 às 12:00 |
Notícias relacionadas: | eso1117 |
Tamanho: | 1832 x 1836 px |
Sobre o objeto
Nome: | Large Magellanic Cloud, LMC, Tarantula Nebula, VFTS 682, Wolf-Rayet Star |
Tipo: | Local Universe : Star : Type : Wolf-Rayet Local Universe : Galaxy : Type : Irregular |
Distância: | 170000 anos-luz |
Constellation: | Dorado |
Categoria: | Star Clusters Stars |
Papéis de parede
Coordenadas
Position (RA): | 5 38 37.98 |
Position (Dec): | -69° 5' 42.18" |
Field of view: | 10.54 x 10.56 arcminutes |
Orientação: | O norte está a 0.2° à direita da vertical |
Cores e filtros
Banda | Comprimento de onda | Telescópio |
---|---|---|
Óptico V | 539 nm | MPG/ESO 2.2-metre telescope WFI |
Infravermelho Y | 1.02 μm | Visible and Infrared Survey Telescope for Astronomy VIRCAM |
Óptico R | 651 nm | MPG/ESO 2.2-metre telescope WFI |
Infravermelho J | 1.25 μm | Visible and Infrared Survey Telescope for Astronomy VIRCAM |
Infravermelho K | 2.15 μm | Visible and Infrared Survey Telescope for Astronomy VIRCAM |