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Photographer is exactly "Image by J. Hibbard"
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Creator:Legacy Astronomical Images
Series:Galaxies Series
Unit:Early-type Unit
Type:Legacy Astronomical Image
Description:VLA atomic hydrogen of the central dominant galaxy of the Fornax Cluster, Fornax A (a.k.a. NGC 1316). The gas is shown as blue contours on an optical image from the Digital Sky Survey. The main body of the Fornax A is typical of early type galaxies, but at fainter light levels the galaxy exhibits a peculiar morphology, with many shells, ripples and loops. The VLA spectral line observations show gas associated with the galaxy NGC 1317 just to the north, the barred galaxy NGC 1310 to the west, and in several small clounds around the main body of NGC 1316. Its possible that the gas clouds are left over from a merger event which fueled the central radio source.
Radio data are VLA DnC-array observations at 54"x43" resolution. HI contours start at a level of 2x10<sup>19</sup> atoms cm<sup>-2</sup>, with successive contours a factor of two higher.
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Creator:Legacy Astronomical Images
Series:Galaxies Series
Unit:Peculiar Unit
Type:Legacy Astronomical Image
Description:A composite image of the optical light (green and yellow) and cold atomic hydrogen gas (blue) in the "Ring Galaxy" Arp 143 (a.k.a. NGC 2444/5). The atomic hydrogen observations, taken with the VLA in its C and D-array configurations, shows a suprising gaseous tidal tails reaching far to the north of this galaxy, to a total distance of 175 kpc or 570,000 light years in length (for Ho=75 km/s/Mpc). There was no hint of this tidal tail in previous optical images. Deeper optical imaging may show a hint of starlight associated with the tail, but it is mostly a gaseous structure. Notice gas also associated with the classical grand-design spiral galaxy to the right
VLA C+D array observations obtained by Appleton et al. (1987), with a resolution of 28". Optical image is R-band image taken by J. Hibbard with the KPNO 0.9m telescope in 10/92.
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