NGC 1275

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:

C. Conselice/Caltech and WIYN/NOIRLab/NSF/AURA

About the Image

Id:noao-n1275
Type:Observation
Release date:July 18, 2005, 9:10 a.m.
Related announcements:noaoann05017
Size:979 x 1321 px

About the Object

Name:NGC 1275
Constellation:Perseus
Category:Galaxies

Image Formats

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761.5 KB
Screensize JPEGScreensize JPEG
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Coordinates

ObjectValue
Position (RA):3 19 47.55
Position (Dec):41° 31' 36.65"
Field of view:3.21 x 4.33 arcminutes
Orientation:North is 0.2° left of vertical


Colors & filters

BandWave-lengthTele-scope
Optical
v
606 nmWIYN 3.5-meter Telescope
Optical
i
780 nmWIYN 3.5-meter Telescope
Optical
H-alpha
656 nmWIYN 3.5-meter Telescope