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 NGC5907 - The Splinter Galaxy 


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NGC5907 Core
Inverted Tidal Tail
KUG1513+566
 

About:
NGC 5907 is a spiral galaxy located approximately 50 million light years from Earth. It has an anomalously low metallicity and few detectable giant stars, being apparently composed almost entirely of dwarf stars. It is a member of the NGC 5866 Group. NGC 5907 has long been considered a prototypical example of a warped spiral in relative isolation. Then in 2006, an international team of astronomers announced the presence of an extended tidal stream surrounding the galaxy and suggests the gravitational perturbations induced by the stream progenitor may be the cause for the warp. NGC 5907 is also known at the Knife Edge or Splinter galaxy. The galaxy was discovered in 1788 by William Herschel. [Text adapted from Wikipedia]



Optics: GSO RC 10" F8 2000mm - Astrograph Ritchie-Chrétien
Mount: AP Mach1 GTO on Gemini Q-Lock tripod
Camera: QSI-640WSG
Filters: Astrodon LRGB 1.25" I Series Gen II
Guiding Systems: SXV-AO-LF Active Optics - SX Lodestar
Dates/Times: 13 May 2013 - 7 June 2013
Location: Pragelato - Turin - (Italy)
Exposure Details: L:R:G:B => 200:48:48:48 = > (20x10):(6x8):(6x8):(6x8) color Bin2 [num x minutes]
Cooling Details: -25°C
Acquisition: Maxim DL/CCD, TheSkyX, Voyager
Processing: CCDStack2+, PS CS5, PI
Mean FWHM: 1.98" / 2.22"
SQM-L: 20.62 / 20.78