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 NGC206 - Star Cloud in Andromeda Galaxy 




Star Cloud
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About:
Nestled within the dusty arms of the large spiral galaxy Andromeda (M31), the star cluster NGC 206 is one of the largest star forming regions known in our local group of galaxies. The beautiful bright blue stars of NGC 206 betray its youth - but close, systematic studies of variable stars in and around NGC 206 will also accurately reveal its distance. Astronomers are searching for variable stars in NGC 206, particularly pulsating stars known as Cepheids and eclipsing binary star systems. Distances for these types of stars can be effectively determined by following the periodic changes in their brightness and spectra. About 3 million light-years away, an accurately known distance to NGC 206 and thus M31 is critical to the larger understanding of galaxy formation, galaxy evolution, and ultimately the distance scale of the Universe. [Text from APOD]

Pubblications "Nuovo Orione" Year 2013 Calendar
Optics: GSO RC 10" F8 2000mm - Astrograph Ritchie-Chrétien
Mount: AP Mach1 GTO on Gemini Q-Lock tripod
Camera: ATIK 4000LE with SX USB Filter Wheel
Filters: Baader LRGB 2"
Guiding Systems: SXV-AO-LF Active Optics - SX Lodestar
Dates/Times: 27/28/29/31 August 2011
Location: Pragelato - Turin - Italy
Exposure Details: L:H:R:G:B => 300:60:70:70:70 = > (30x10):(2x30):(14x5):(14x5):(14x5) Color Bin2 [num x minutes]
Cooling Details: -20 °C
Acquisition: Maxim DL/CCD, Perseus
Processing: CCDStack2, PixInsight, PS CS2
Mean FWHM: 1.68 / 2.21 "
SQM-L: 21.13 / 21.31