II* F L X 4 d l ( 1 t 2 ; = # A ) j ) I x; / i 8m s 0 k Galaxy NGC 7793, located approximately 10 million light-years away, is a member of the Sculptor group of galaxies. This galaxy cluster, named after the constellation in which it resides, is one of the closest to our own Local Group of galaxies. This image was captured as part of the Spitzer Infrared Nearby Galaxy Survey (SINGS) Legacy Project using the telescope's Infrared Array Camera (IRAC).
As the "glowing" red emission maps out, Spitzer is able to pierce through dense clouds of gas and dust that comprise the spiral disk, revealing new star formation that is driving the evolution of the galaxy.
The SINGS image is a four channel false color composite, where blue indicates emission at 3.6 microns, green corresponds to 4.5 microns, and red to 5.8 and 8.0 microns. The contribution from starlight (measured at 3.6 microns) in this picture has been subtracted from the 5.8 and 8 micron images to enhance the visibility of the dust features. bm F N] + [ o E Q / P< / a - ' - ' Adobe Photoshop CS3 Macintosh 2008:11:11 13:06:09 Spitzer Space Telescope
Pasadena
USA
1200 E. California Blvd.
91125
CA
http://www.spitzer.caltech.edu
Distance from Quickfacts. Redshift from NED 2008/11/11
10000000
0.000757
Spitzer
Spitzer
Spitzer
Spitzer
sig05-017
Good
IRAC
IRAC
IRAC
IRAC
2012-10-11
1.1
Spitzer Science Center
spitzer
http://www.spitzer.caltech.edu/images/2371-sig05-017-NGC-7793
sig05-017.tif
http://www.spitzer.caltech.edu/uploaded_files/images/0001/3501/sig05-017.tif
ICRS
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J2000
Full
990
990
220.051364899
870.036046982
359.437714616
-32.6868311765
-152.64294901139
-0.00020908552099377
0.00020908552099377
Infrared
Infrared
Infrared
Infrared
Near-IR
Near-IR
Mid-IR
Mid-IR
3600
4500
5800
8000
Blue
Green
Red
Red
The contribution from starlight has been subtracted from the 5.8 and 8.0 micron channels to enhance the visibility of dust features.
C.5.1.1.
C.5.3.3
Observation
Spitzer Space Telescope
Galaxy NGC 7793, located approximately 10 million light-years away, is a member of the Sculptor group of galaxies. This galaxy cluster, named after the constellation in which it resides, is one of the closest to our own Local Group of galaxies. This image was captured as part of the Spitzer Infrared Nearby Galaxy Survey (SINGS) Legacy Project using the telescope's Infrared Array Camera (IRAC).
As the "glowing" red emission maps out, Spitzer is able to pierce through dense clouds of gas and dust that comprise the spiral disk, revealing new star formation that is driving the evolution of the galaxy.
The SINGS image is a four channel color composite, where blue indicates emission at 3.6 microns, green corresponds to 4.5 microns, and red to 5.8 and 8.0 microns. The contribution from starlight (measured at 3.6 microns) in this picture has been subtracted from the 5.8 and 8 micron images to enhance the visibility of the dust features.
NGC 7793
NGC 7793
NASA/JPL-Caltech/R. Kennicutt (University of Arizona) and the SINGS legacy team
2005-09-15
Galaxy NGC 7793, located approximately 10 million light-years away, is a member of the Sculptor group of galaxies. This galaxy cluster, named after the constellation in which it resides, is one of the closest to our own Local Group of galaxies. This image was captured as part of the Spitzer Infrared Nearby Galaxy Survey (SINGS) Legacy Project using the telescope's Infrared Array Camera (IRAC).
Spitzer Space Telescope
http://www.spitzer.caltech.edu/info/18-Image-Use-Policy
http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml Z %G xGalaxy NGC 7793, located approximately 10 million light-years away, is a member of the Sculptor group of galaxies. This galaxy cluster, named after the constellation in which it resides, is one of the closest to our own Local Group of galaxies. This image was captured as part of the Spitzer Infrared Nearby Galaxy Survey (SINGS) Legacy Project using the telescope's Infrared Array Camera (IRAC).
As the "glowing" red emission maps out, Spitzer is able to pierce through dense clouds of gas and dust that comprise the spiral disk, revealing new star formation that is driving the evolution of the galaxy.
The SINGS image is a four channel false color composite, where blue indicates emission at 3.6 microns, green corresponds to 4.5 microns, and red to 5.8 and 8.0 microns. The contribution from starlight (measured at 3.6 microns) in this picture has been subtracted from the 5.8 and 8 micron images to enhance the visibility of the dust features.i Galaxy NGC 7793, located approximately 10 million light-years away, is a member of the Sculptor group of galaxies. This galaxy cluster, named after the constellation in which it resides, is one of the closest to our own Local Group of galaxies. This imageP Spitzer Space Telescopen NASA/JPL-Caltech/R. Kennicutt (s Spitzer Space Telescope NGC 77937 20050915 NGC 7793t @http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml 8BIM Z %G xGalaxy NGC 7793, located approximately 10 million light-years away, is a member of the Sculptor group of galaxies. This galaxy cluster, named after the constellation in which it resides, is one of the closest to our own Local Group of galaxies. This image was captured as part of the Spitzer Infrared Nearby Galaxy Survey (SINGS) Legacy Project using the telescope's Infrared Array Camera (IRAC).
As the "glowing" red emission maps out, Spitzer is able to pierce through dense clouds of gas and dust that comprise the spiral disk, revealing new star formation that is driving the evolution of the galaxy.
The SINGS image is a four channel false color composite, where blue indicates emission at 3.6 microns, green corresponds to 4.5 microns, and red to 5.8 and 8.0 microns. The contribution from starlight (measured at 3.6 microns) in this picture has been subtracted from the 5.8 and 8 micron images to enhance the visibility of the dust features.i Galaxy NGC 7793, located approximately 10 million light-years away, is a member of the Sculptor group of galaxies. This galaxy cluster, named after the constellation in which it resides, is one of the closest to our own Local Group of galaxies. This imageP Spitzer Space Telescopen NASA/JPL-Caltech/R. Kennicutt (s Spitzer Space Telescope NGC 77937 20050915 NGC 7793t @http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml8BIM% ͕X22 :8BIM
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