The Hydrogen Gas Disk in M33 |
 | Minimum credit line: Image courtesy of NRAO/AUI
(for details, see .
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The distribution of the cold neutral atomic hydrogen gas in the Scd
galaxy Messier 33, also known as the "Triangulum Galaxy". Bright
regions indicate regions with a high gas density, while dark regions
have little or no gas. The underlying stellar disk of this galaxy
is not shown, but appears elsewhere in the image gallery. This image
emphasizes the wealth of structure present in the gas disk, from
tight knots of gas associated with star forming regions, to
large holes which may have been swept clean of gas by the winds
from massive stars or by exploding supernovae.
Investigator(s): David Thilker, Robert Braun, and Rene Walterbos This image is available in the following downloadable versions: If you would like to obtain a higher resolution version of this image,
please contact .
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Telescope
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ALMA
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Date of Observation
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1998-08-15
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Type of Observation
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Spectral Line Observations
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Wavelength
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21 cm
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Frequency
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1420.4 MHz
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Species
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HI
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Center of Image
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RA: 01:33:51.02, Dec: 30:39:36.70 (J2000)
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Field of View
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1.0000 x 1.0000 degrees
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Technical Caption
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The data were obtained from VLA observations taken both in its B-array
and CS-array configurations, with a spatial resolution of 10" and
velocity resolution of 1.3 km/s. The VLA data have been supplemented
by total power observations obtained at the Westerbork Synthesis Radio
Telescope.
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