Atomic Gas in the NGC 5018 Group |
 | Minimum credit line: Image courtesy of NRAO/AUI
(for details, see .
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VLA atomic hydrogen observations of the NGC 5018 group. The upper
panel is the optical image from the Digital Sky
Survey, while the lower panel shows the same optical image to
fainter light levels, with contours indicating the distribution of the
cold atomic gas. NGC 5018 is classified as a normal E3 elliptical
galaxy, but at fainter light levels the galaxy exhibits a peculiar
morphology, with many shells, ripples and loops. The VLA spectral line
observations shows gas associated with a number of spiral galaxies in
the group, and a few clouds which are not apparently associated with
any optically identified system. Most interestingly, there is an
extended gas "bridge" of material connecting two spirals on
either side of NGC 5018, and the gaseous bridge appears to bend to
avoid the elliptical. Investigator(s): P. Guhathakurta, J. van Gorkom, G. Knapp & D.-W Kim. Composite image by J. Hibbard This image is available in the following downloadable versions: If you would like to obtain a higher resolution version of this image,
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Telescope
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VLA
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Date of Observation
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1987-05-13
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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: 13:13:5.50, Dec: -19:28:28.00 (J2000)
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Field of View
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0.4667 x 0.4333 degrees
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Technical Caption
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Radio data are VLA D-array observations at 60"
resolution. HI contours start at a level of 3x1019
atoms cm-2,
with successive contours a factor of two higher.
Earlier versions of this data was published in
Kim et al. 1988.
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