Spiral galaxy NGC4013
credit line: C. Howk (JHU), B. Savage (U. Wisconsin), N.A.Sharp (NOAO)/WIYN/NOAO/NSFÂ
NOAO

seen from United States
seen from Malaysia

seen from Iraq

seen from Malaysia
seen from Türkiye
seen from Germany

seen from Malaysia
seen from Netherlands
seen from United States

seen from Türkiye
seen from South Africa
seen from Indonesia
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seen from Russia
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seen from France

seen from United Kingdom

seen from United States
seen from Malaysia
seen from United States
Spiral galaxy NGC4013
credit line: C. Howk (JHU), B. Savage (U. Wisconsin), N.A.Sharp (NOAO)/WIYN/NOAO/NSFÂ
NOAO

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M83 [NGC5236] Southern Pinwheel [NOAO Telescope]
O telescópio Blanco no observatório do CTIO, Chile. . Blanco telescope at CTIO Observatory, Chile. . Credit: DES . #des #blanco #telescope #telescopio #astronomy #astronomia #observatoriog1 #astrogram #chile #noao #ctio #tololo #milkyway #vialactea
Spiral Galaxy NGC4402
Minimum credit line: H.Crowl (Yale University) and WIYN/NOAO/AURA/NSF
NOAO
Spiral Galaxy NGC 4395
This image was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory.
credit line: T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOAO/AURA/NSF)
NOAO

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Dwarf Galay NGC 4214
This image was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory.
credit line: T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOAO/AURA/NSF)
NOAO
NGC1512/10, SINGG Survey
This image shows a strong interaction between the barred spiral NGC1512 and its Blue Compact Dwarf (BCD) companion, NGC1510. Star formation in NGC1512 is concentrated into two rings; the inner one has the strength of a starburst. Surprisingly star formation is even stronger in the BCD NGC1510, which can be seen to the lower right of NGC1512. This pair ilustrate how galaxy interactions are able to trigger starbursts.
credit line: The SINGG Survey Team and NOAO/AURA/NSF
NOAO
NGC1275
This image shows a deep Hydrogen-alpha image of the brightest X-ray source in the sky, NGC1275, taken by the WIYN 3.5-meter telescope at Kitt Peak National Observatory near Tucson, AZ, in 1999.
The filaments emanating from this galaxy are produced through largely unknown mechanisms, but they likely are the result of an interaction between the black hole in the center of the galaxy and the intracluster medium surrounding it. (The glowing background objects in this image are galaxies in that same galaxy cluster.)
At a distance of about 230 million light-years, this is the nearest example to Earth of such vast structures, which are seen surrounding the most massive galaxies throughout the Universe.
credit line: C. Conselice/Caltech and WIYN/NOAO/AURA/NSF
NOAO