Neutral Gas Disk of the Milky Way
Description
This figure shows the distribution of atomic hydrogen at all locations in the sky. All of this hydrogen is in our galaxy. Red indicates directions of high hydrogen density, blue and black show areas with little hydrogen. The figure is centered on the galactic center and galactic longitude increases to the left. The data came from measurements of the 21cm line of hydrogen by radio telescopes. Some of the hydrogen loops outline old supernova remnants. This image is a composite from many 21cm surveys. It includes data from the NRAO Green Bank, West Virginia 140- foot and 300-foot telescopes, the 85-foot Hat Creek Telescope of The University of California at Berkeley, The AT&T Bell-Labs Horn-Reflector Telescope at Holmdel, New Jersey and The 60-foot Telescope at the Parkes Radio Observatory in Australia.
Creator
Legacy Astronomical Images
Rights
NRAO/AUI/NSF does not hold full copyright for this image. Contact the archivist for details.
Type
Legacy Astronomical Image
Object Name
Milky Way
Investigators
J.M. Dickey, F.J. Lockman
Telescope
140 Foot Telescope
300 Foot Telescope
Hat Creek Telescope
Horn-Reflector Telescopes
60 Foot Parkes Telescope
Type of Observation
spectral line
Wavelength
21 cm
Frequency
1420.4 MHz
Species
HI
Center of Image
RA 26:0:0.000, Dec: 0:0:0.000
Field of View
360.000000 x 360.000000 degrees
Link to journal article
Notes
Contact the archivist for a high resolution tif of this image.
Series
Galaxies Series
Unit
Spiral Unit
Citation
Legacy Astronomical Images, “Neutral Gas Disk of the Milky Way,” NRAO/AUI Archives, accessed December 20, 2024, https://www.nrao.edu/archives/items/show/33582.