Astroman
13-09-2015, 10:06 AM
NGC-253 again. This time with 4hrs of data. 50 x 300sec exposures, ISO800. Canon 1100D (unmodded), 8" f/4 Newtonian. Has slight focus shift during the imaging run, which may have affected the overall sharpness of the galaxy.
Larger Image : http://www.astrobin.com/full/210315/0/
The galaxy was discovered by Caroline Herschel in 1783 during one of her systematic comet searches.[4][5] About half a century later, John Herschel observed it using his 18-inch metallic mirror reflector at the Cape of Good Hope.[5] He wrote, "very bright and large (24′ in length); a superb object.... Its light is somewhat streaky, but I see no stars in it except 4 large and one very small one, and these seem not to belong to it, there being many near..."[5]
In 1961 Allan Sandage wrote in the Hubble Atlas of Galaxies that the Sculptor Galaxy is "the prototype example of a special subgroup of Sc systems....photographic images of galaxies of the group are dominated by the dust pattern. Dust lanes and patches of great complexity are scattered throughout the surface. Spiral arms are often difficult to trace.... The arms are defined as much by the dust as by the spiral pattern."[6] Bernard Y. Mills, working out of Sydney, discovered that the Sculptor Galaxy is also a fairly strong radio source.[5]
In 1998 the Hubble Space Telescope took a detailed image of NGC 253.[7]
Larger Image : http://www.astrobin.com/full/210315/0/
The galaxy was discovered by Caroline Herschel in 1783 during one of her systematic comet searches.[4][5] About half a century later, John Herschel observed it using his 18-inch metallic mirror reflector at the Cape of Good Hope.[5] He wrote, "very bright and large (24′ in length); a superb object.... Its light is somewhat streaky, but I see no stars in it except 4 large and one very small one, and these seem not to belong to it, there being many near..."[5]
In 1961 Allan Sandage wrote in the Hubble Atlas of Galaxies that the Sculptor Galaxy is "the prototype example of a special subgroup of Sc systems....photographic images of galaxies of the group are dominated by the dust pattern. Dust lanes and patches of great complexity are scattered throughout the surface. Spiral arms are often difficult to trace.... The arms are defined as much by the dust as by the spiral pattern."[6] Bernard Y. Mills, working out of Sydney, discovered that the Sculptor Galaxy is also a fairly strong radio source.[5]
In 1998 the Hubble Space Telescope took a detailed image of NGC 253.[7]