The brilliant star VFTS 682 in the Large Magellanic Cloud (annotated)
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 upper left is the brilliant but isolated star VFTS 682 and at the lower right is 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.
Źródło:ESO/M.-R. Cioni/VISTA Magellanic Cloud survey. Acknowledgment: Cambridge Astronomical Survey Unit
O zdjęciu
Identyfikator: | eso1117b |
Typ: | Obserwacje |
Data publikacji: | 25 maja 2011 12:00 |
Powiązane komunikaty: | eso1117 |
Rozmiar: | 622 x 858 px |
O obiekcie
Nazwa: | VFTS 682 |
Typ: | Local Universe : Star : Type : Wolf-Rayet |
Odległość: | 170000 lat świetlnych |
Constellation: | Dorado |
Kategoria: | Nebulae Star Clusters |
Współrzędne
Pozycja (RA): | 5 38 42.61 |
Pozycja (Dec): | -69° 6' 3.89" |
Kolory i filtry
Pasmo | Teleskop |
---|---|
Optyczny V | MPG/ESO 2.2-metre telescope WFI |
Podczerwony Y | Visible and Infrared Survey Telescope for Astronomy |
Optyczny R | MPG/ESO 2.2-metre telescope WFI |
Podczerwony J | Visible and Infrared Survey Telescope for Astronomy |
Podczerwony K | Visible and Infrared Survey Telescope for Astronomy |