M82, Cigar Galaxy

8мар

Messier 82 (also known as NGC 3034, Cigar Galaxy or M82) is a starburst galaxy about 12 million light-years away in the constellation Ursa Major. It is about five times more luminous than the whole Milky Way and one hundred times more luminous than our galaxy’s center. The starburst activity is thought to be triggered by interaction with neighboring galaxy M81, and M82 is a member of the M81 Group. As the closest starburst galaxy to our own, M82 is the prototypical example of this type of galaxy. SN 2014J, a Type Ia supernova, was observed in the galaxy on 21 January 2014. In 2014, in studying M82, scientists discovered the brightest pulsar yet known, designated M82 X-2.

  • Imaging telescopes or lenses: SLOOH T2HM C14″ f/11
  • Imaging cameras: SBIG ST-10XME
  • Software: Pixinsight 1.8
  • Filters: Luminance,  Blue,  Green,  Red
  • Resolution: 3360×2612
  • Frames:
    Blue: 205×20″ -10C bin 3×3
    Green: 212×20″ -10C bin 3×3
    Luminance: 173×50″ -10C bin 2×2
    Red: 207×20″ ISO20 -10C bin 3×3
  • Integration: 5.9 hours
  • Darks: ~14
  • Bias: ~2
  • RA center: 148.987 degrees
  • DEC center: 69.696 degrees
  • Pixel scale: 0.233 arcsec/pixel
  • Orientation: 179.846 degrees
  • Field radius: 0.138 degrees
  • Locations: SLOOH Teide, Canary Islands, Mt. Teide, Canary Islands, Spain

Author: Peter Ilas

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