Dwarf Galaxy UGC 5391 |
 | Minimum credit line: Image courtesy of NRAO/AUI
(for details, see .
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A collection of radio and optical images of the dwarf spiral galaxy
UGC 5391. Clockwise (from the upper left panel) are the distribution of total atomic hydrogen (HI) shown as contours and greyscales; the
velocity distribution of the HI contoured upon the total HI map; color-coded HI velocity field (red indicates gas which is moving away from us, blue gas which is moving towards us); and the total HI map contoured upon an optical image from the
Digital Sky Survey. Investigator(s): E. M. Wilcots and M. K. Prescott This image is available in the following downloadable versions:
- 532 x 648
- 1064 x 1297
- 0 x 0
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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2002-00-00
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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: 10:01:41.11, Dec: 37:14:51.90 (J2000)
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Field of View
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0.3000 x 0.3000 degrees
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Technical Caption
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Contour levels on the total HI maps are 0.13, 0.25, 0.5, 1.0, and 1.8 x 1020 cm-2. The gray scales in the first two panels are in units of 1020 cm-2. The color-coded velocity scale in panel 3 is in units of kilometers per second.
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- Astronomical database entries for UGC5391
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