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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.
Oikeudet:ESO/M.-R. Cioni/VISTA Magellanic Cloud survey. Acknowledgment: Cambridge Astronomical Survey Unit
Kuvasta
| Tunnistus: | eso1117a |
| Tyyppi: | Havainto |
| Julkaisupäivä: | 25. toukokuuta 2011 12:00 |
| Vastaavat julkaisut: | eso1117 |
| Koko: | 1832 x 1836 px |
Kohteesta
| Nimi: | Large Magellanic Cloud, LMC, Tarantula Nebula, VFTS 682, Wolf-Rayet Star |
| Tyyppi: | Local Universe : Star : Type : Wolf-Rayet Local Universe : Galaxy : Type : Irregular |
| Etäisyys: | 170000 valovuotta |
| Constellation: | Dorado |
| Kategoria: | Star Clusters Stars |
Taustakuvat
Koordinaatit
| Position (RA): | 5 38 37.98 |
| Position (Dec): | -69° 5' 42.18" |
| Field of view: | 10.54 x 10.56 arcminutes |
| Suuntaus: | Pohjoinen on 0.2° oikea pystysuuntaan nähden |
Katso WorldWide Telescope:ssa:
Värit ja suotimet
| Kaista | Aallonpituus | Teleskooppi |
|---|---|---|
| Optinen V | 539 nm | MPG/ESO 2.2-metre telescope WFI |
| Infrapuna Y | 1.02 μm | Visible and Infrared Survey Telescope for Astronomy VIRCAM |
| Optinen R | 651 nm | MPG/ESO 2.2-metre telescope WFI |
| Infrapuna J | 1.25 μm | Visible and Infrared Survey Telescope for Astronomy VIRCAM |
| Infrapuna K | 2.15 μm | Visible and Infrared Survey Telescope for Astronomy VIRCAM |