Fayl:Phot-20d-99-hires.jpg

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Asl fayl ‎(2 045 × 2 037 piksel, fayl hajmi: 4,23 MB, MIME tipi: image/jpeg)

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English: A pair of galaxies NGC 5090 - 5091 in Centaurus is shown in this image. They are located at about the same distance as ESO 269-57 and may belong to the same cluster of galaxies. This is an interacting elliptical-spiral system with some evidence of tidal disruption of NGC 5091 (to the left; seen under a steep angle) by NGC 5090 (to the right). The velocity of the nucleus of NGC 5091 has been measured as 3429 km/sec, while NGC 5090 has a velocity of 3185 km/sec. NGC 5090 is associated with a strong, double radio source (PKS 1318-43). This three-colour composite (BVR) was obtained with VLT UT1/ANTU and its FORS1 instrument in the morning of March 29, 1999. A bright star in the Milky Way, just outside the field at the upper left, has produced a pattern of blue straylight. The field size is 6.8x6.8 arcmin 2. North is up and East is to the left.
Sanasi Taken on 29 Mart 1999
Manba http://www.eso.org/outreach/press-rel/pr-1999/phot-20-99.html (archived; image link); see also https://www.eso.org/public/images/eso9924d/
Muallif European Southern Observatory
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  • atribut – Siz tegishli litsenziyaga havolani taqdim etishingiz va oʻzgartirishlar kiritilganligini koʻrsatishingiz kerak. Siz buni har qanday oqilona yoʻl bilan qilishingiz mumkin, lekin litsenziar Sizni yoki Sizning foydalanishingizni ma'qullashini taklif qiladigan tarzda emas.

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29 Mart 1999

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Faylning biror paytdagi holatini koʻrish uchun tegishli sana/vaqtga bosingiz.

Sana/VaqtMiniaturaOʻlchamlariFoydalanuvchiIzoh
joriy16:18, 2-May 200916:18, 2-May 2009 dagi versiya uchun tasvir2 045 × 2 037 (4,23 MB)Fabian RRRR{{Information |Description={{en|1=A pair of galaxies NGC 5090 - 5091 in Centaurus is shown in this image. They are located at about the same distance as ESO 269-57 and may belong to the same cluster of galaxies. This is an interacting elliptical-spiral sy

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Metama’lumot

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"https://uz.wikipedia.org/wiki/Fayl:Phot-20d-99-hires.jpg" dan olindi