MM * 4 4 : @ 4 \ ) 4 , ( 1 2 (; ! <= # ^ * HI Z _i rs H r This composite image of X-ray (red), radio (dark blue), and optical (light blue) data shows activity from the central black hole in 3C305. Unexpectedly, Chandra's X-ray data do not appear to align with radio emission detected by the Very Large Array, but do overlap with the optical emission. Using this information, astronomers believe the X-ray emission is caused either by jets or radiation surrounding the black hole. One of these mechanisms is infusing the interstellar gas with enough energy to cause it to glow in X-ray light. ht. > ` T V * N d `
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Log(x)
0.02266808971763
4.57791423797607
0.00000000000000
500.00000000000000
0.00000000000000
2.43408188707942
592000000
Chandra
Hubble
VLA
ACIS
WFPC2
-
Red
Cyan
Blue
X-ray
Optical
Radio
-
FR533N
L-band
0.8267
-
2e8
2008-04-07T10:23:21
-
-
7800
-
-
C.5.4.6
222.3401756
63.2705950
2100.0
2100.0
1051.0
1051.0
4.57378e-06
4.573779e-06
WCS retrieved using CXCs PinpointWCS
9330
-
-
An Intriguing Glowing Galaxy
3C305
Chandra X-ray Observatory Center
This composite image of X-ray (red), radio (dark blue), and optical (light blue) data shows activity from the central black hole in 3C305. Unexpectedly, Chandra's X-ray data do not appear to align with radio emission detected by the Very Large Array, but do overlap with the optical emission. Using this information, astronomers believe the X-ray emission is caused either by jets or radiation surrounding the black hole. One of these mechanisms is infusing the interstellar gas with enough energy to cause it to glow in X-ray light.
http://chandra.harvard.edu/photo/image_use.html
pCore:CreatorContactInfo rdf:parseType="Resource">
http://chandra.harvard.edu
cxcpub@cfa.harvard.edu
617.496.7941
60 Garden St.
Cambridge
MA
02138
USA
http://chandra.harvard.edu/photo/image_use.html
xThis composite image of X-ray (red), radio (dark blue), and optical (light blue) data shows activity from the central black hole in 3C305. Unexpectedly, Chandra's X-ray data does not appear to align with radio emission detected by the Very Large Array, but does overlap with the optical emission. Using this information, astronomers believe the X-ray emission is caused either by jets or radiation surrounding the black hole. One of these mechanisms is infusing the interstellar gas with enough energy to cause it to glow in X-ray light.i [A galaxy, about 600 million light years away, with a supermassive black hole at its center.P Chandra X-ray Observatory Centern X-ray (NASA/CXC/CfA/F.Massaro, es Chandra X-ray Observatory An Intriguing Glowing Galaxy7 20090514 3C305 8BIM , , 8BIM 8BIM H /ff lff /ff 2 Z 5 - 8BIM p 8BIM & xThis composite image of X-ray (red), radio (dark blue), and optical (light blue) data shows activity from the central black hole in 3C305. Unexpectedly, Chandra's X-ray data does not appear to align with radio emission detected by the Very Large Array, but does overlap with the optical emission. Using this information, astronomers believe the X-ray emission is caused either by jets or radiation surrounding the black hole. One of these mechanisms is infusing the interstellar gas with enough energy to cause it to glow in X-ray light.i [A galaxy, about 600 million light years away, with a supermassive black hole at its center.P Chandra X-ray Observatory Centern X-ray (NASA/CXC/CfA/F.Massaro, es Chandra X-ray Observatory An Intriguing Glowing Galaxy7 20090514 3C3058BIM @ @ 8BIM % , JFIF H H Adobe_CM Adobe d
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