Dosya:ESO Centaurus A LABOCA.jpg

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Ebato oricinale(2,808 × 2,957 pikselan, ebatê dosya: 5.18 MB, MIME tipê cı: image/jpeg)


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Şınasnayış
العربية: صُورة مُركبة مُلونة لِمجرَّة قنطورس A، تكشف الفُصُوص والانبعاثات الصادرة من الثُقب الأسود النشط في قلب هذه المجرَّة. رُكِّبت هذه الصُورة من مججموعةٍ من الصُور التي حصل عليها العُلماء بِواسطة ثلاثة أدوات، يعملُ كُلٌ منها على طول موجاتٍ مُختلفةٍ عن الأُخرى.
English: Colour composite image of Centaurus A, revealing the lobes and jets emanating from the active galaxy’s central black hole. This is a composite of images obtained with three instruments, operating at very different wavelengths. The 870-micron submillimetre data, from LABOCA on APEX, are shown in orange. X-ray data from the Chandra X-ray Observatory are shown in blue. Visible light data from the Wide Field Imager (WFI) on the MPG/ESO 2.2 m telescope located at La Silla, Chile, show the background stars and the galaxy’s characteristic dust lane in close to "true colour".
Tarix (released)
Çıme http://www.eso.org/public/images/eso0903a/
Nuştekar ESO/WFI (Optical); MPIfR/ESO/APEX/A.Weiss et al. (Submillimetre); NASA/CXC/CfA/R.Kraft et al. (X-ray)
Destur
(Reyna sixulnayise ena dosya)
http://www.eso.org/public/outreach/press-rel/copyright.html
Versiyonane binan
 Black Hole Outflows From Centaurus A.jpg

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Dewrê mocnayışi

28 Çele 2009

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nıkayên09:03, 27 Keşkelun 2012Seba versiyonê 09:03, 27 Keşkelun 2012 ra2,808 - 2,957 (5.18 MB)PineLarger version. The original filename of the larger version was "eso0903a.tif". I changed it to a JPG to reduce the file size and maintain the same file format as the previous versions since Commons requires the updated file to use the same filename as...
20:08, 29 Çele 2009Seba versiyonê 20:08, 29 Çele 2009 ra1,600 - 1,564 (409 KB)HorsePunchKid{{Information |Description={{en|1=Colour composite image of Centaurus A, revealing the lobes and jets emanating from the active galaxy’s central black hole. This is a composite of images obtained with three instruments, operating at very different wavel

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