NASA's Chandra Observatory Identifies Impact of Cosmic Chaos on Star Birth

Chandra_582a_1024

chandra_582a October 27th, 2014

Credit: NASA/CXC/Stanford/I.Zhuravleva et al

Chandra observations of the Perseus and Virgo galaxy clusters have provided direct evidence that turbulence is helping to prevent stars from forming there. These new results could answer a long-standing question about how these galaxy clusters keep their enormous reservoirs of hot gas from cooling down to form stars. Scientists targeted Perseus and Virgo because they are both extremely large and relatively bright, thus providing an opportunity to see details that would be very difficult to detect in other clusters.

Provider: Chandra X-ray Observatory

Image Source: http://chandra.harvard.edu/photo/2014/perseusvirgo/

Curator: Chandra X-ray Observatory, Cambridge, MA, USA

Image Use Policy: http://chandra.harvard.edu/photo/image_use.html

Image Details

Image Type
Observation
Object Name
Perseus Cluster
Subject - Local Universe
Galaxy > Grouping > Cluster

Distance

Universescale3
250,000,000 light years
Chandra_582a_128
 

Position Details

Position (ICRS)
RA = 3h 19m 48.1s
DEC = 41° 30’ 42.6”
Orientation
North is up
Field of View
19.8 x 19.8 arcminutes
Constellation
Perseus

Color Mapping

  Telescope Spectral Band Wavelength
Purple Chandra (ACIS) X-ray (X-ray) 826.7 pm
Spectrum_xray1
Purple
Chandra_582a_1280
×
ID
582a
Subject Category
C.5.5.3  
Subject Name
Perseus Cluster
Credits
NASA/CXC/Stanford/I.Zhuravleva et al
Release Date
2014-10-27
Lightyears
250,000,000
Redshift
250,000,000
Reference Url
http://chandra.harvard.edu/photo/2014/perseusvirgo/
Type
Observation
Image Quality
Good
Distance Notes
Facility
Chandra
Instrument
ACIS
Color Assignment
Purple
Band
X-ray
Bandpass
X-ray
Central Wavelength
0.8267
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
J2000
Reference Value
49.9504617, 41.5118326
Reference Dimension
3600.0, 3600.0
Reference Pixel
1801.0, 1801.0
Scale
9.17366e-05, 9.1736608e-05
Rotation
0.01
Coordinate System Projection:
TAN
Quality
Full
FITS Header
Notes
WCS retrieved using CXCs PinpointWCS
Creator (Curator)
Chandra X-ray Observatory
URL
http://chandra.harvard.edu
Name
Chandra X-ray Observatory Center
Email
cxcpub@cfa.harvard.edu
Telephone
617.496.7941
Address
60 Garden St.
City
Cambridge
State/Province
MA
Postal Code
02138
Country
USA
Rights
http://chandra.harvard.edu/photo/image_use.html
Publisher
Chandra X-ray Observatory Center
Publisher ID
chandra
Resource ID
perseus.tif
Metadata Date
2014-11-20T10:17:51-05:00
Metadata Version
1.2
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Detailed color mapping information coming soon...

×
Universescalefull
250,000,000 light years

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