Fayl:ESP- Big Stellar Cluster in the Blue Dwarf Galaxy NGC 5253-phot-31a-04-fullres.jpg
Bu prevyuning hajmi: 597 × 599 piksel. Boshqa oʻlchamlari: 2 289 × 2 297 piksel.
Asl fayl (2 289 × 2 297 piksel, fayl hajmi: 1,51 MB, MIME tipi: image/jpeg)
Qisqa izoh
| Taʼrif |
English: Composite colour-coded image of the small starburst galaxy NGC 5253, at a distance of 11 million light-years. It is based on one near-infrared image (in the K-band at wavelength 2.16 μm; here coded red) obtained with the ESO Very Large Telescope (VLT) and two images in the visual spectral region (V- (0.55 μm) and I-bands (0.79 μm), here blue and green, respectively) with the NASA/ESA Hubble Space Telescope (HST). The image covers 80 x 80 square arcseconds on the sky. North is up and East is to the left. |
| Sanasi | |
| Manba | http://www.eso.org/gallery/v/ESOPIA/StarClusters/phot-31a-04-fullres.jpg.html |
| Muallif | ESO/NASA/ESA |
| Ruxsat (Bu faylning takror foydalanilishi) |
http://www.eso.org/public/outreach/press-rel/copyright.html |
Search for more ESO images at: http://www.eso.org/gallery/v/ESOPIA
Litsenziyalash
This file is licensed under the Creative Commons Attribution 3.0 Unported license.
- Siz erkinsiz:
- ulashishga – ishlanmani nusxalash, tarqatish va uzatish
- remiks qilishga – ishni moslashtirishga
- Quyidagi shartlar asosida:
- 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.
Fayl tarixi
Faylning biror paytdagi holatini koʻrish uchun tegishli sana/vaqtga bosingiz.
| Sana/Vaqt | Miniatura | Oʻlchamlari | Foydalanuvchi | Izoh | |
|---|---|---|---|---|---|
| joriy | 19:00, 2009-yil 26-iyun | | 2 289 × 2 297 (1,51 MB) | wikimediacommons>Lars Lindberg Christensen | {{Information |Description={{en|1=Composite colour-coded image of the small starburst galaxy NGC 5253, at a distance of 11 million light-years. It is based on one near-infrared image (in the K-band at wavelength 2.16 μm; here coded red) obtained with the |
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