Dates:Feb. 25, 2017 , Feb. 26, 2017 , Feb. 27, 2017
Frames:
Baader Planetarium B 36mm: 35x450" bin 2x2
Baader Planetarium G 36mm: 33x450" bin 2x2
Baader Planetarium L 36mm: 71x900" bin 1x1
Baader Planetarium R 36mm: 34x450" bin 2x2
Integration: 30.5 hours
Avg. Moon age: 19.56 days
Avg. Moon phase: 0.83%
Astrometry.net job: 1479123
RA center: 10h 28' 23"
DEC center: +68° 25' 26"
Pixel scale: 0.957 arcsec/pixel
Orientation: 183.534 degrees
Field radius: 0.357 degrees
Resolution: 1900x1900
Locations: Observatorio remoto Tomas Lopez en AstroCamp, Nerpio, Albacete, Spain
Data source: Own remote observatory
Remote source: AstroCamp
IC 2574 discovered by Edwin Coddington in 1898 and classified first as a nebula is actually a dwarf irregular galaxy in the constellation Ursa Major and is part of the M81 group of galaxies. This long exposure image of this classification type SAB(s)m shows two very dim arms and irregular shape. To the north (top left) is an area of massive star formations surrounded by interstellar medium (ISM) and thought to be triggered by the central stellar cluster and because if its large size it is classified as a 'Super Giant Shell' (SGS).
An extract taken from a study by S. Steward & F. Walter 2000: In the standard picture (e.g., Weaver et al. 1977; McKee & Ostriker 1977; Chu et al.1995), these structures are believed to be created by young star-forming regions that supposedly eject a great amount of mechanical energy into the ambient ISM in terms of strong stellar winds and subsequent supernova (SN) explosions.
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