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| Name / Constellation | NGC 2146 |
Other: 4C +78.06, IRAS 06106+7822, UGC 3429, MCG +13-05-022, PGC 18797, CGCG 348-017 | Cam |
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| Coordinates | AR: 06h 18m 37.71s, +78° 21′ 25.2″ | |||
| Optics | Officina Stellare 10" f8 Richtey-Cretien | |||
| Camera-Mount | PLAYERONE POSEIDON M-PRO - ZWO ASI 1600M (ONAG)- 10Micron GM2000 QCI Mount | |||
| Filters | Antlia V-Pro LRGB | |||
| Exposure |
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| Location / Date | Promiod (Valle D'Aosta-Italy) "TLP" Remote Observatory - Oct/Nov 2024 | |||
| Seeing | 2.2" @ 1.17 arcosec/pixel binning 3 | |||
| Note | Drizzle 2X in postprocessing (Pixinsight)) | |||
| Acquisition | N.I.N.A. | |||
| Processing | Adobe Photoshop CC - |
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| Comment |
NGC 2146 (also known as the Dusty Hand Galaxy) is a barred spiral galaxy type SB(s)ab pec in the constellation Camelopardalis. The galaxy was discovered in 1876 by Friedrich August Theodor Winnecke. It has a diameter of 80,000 lyr. The galaxy's most conspicuous feature is the dusty lanes of a spiral arm lying across the core of the galaxy as seen from Earth, the arm having been bent 45 degrees by a close encounter with a smaller galaxy possibly NGC 2146a about 0.8 billion years ago. This close encounter is credited with the relatively high rates of star formation that qualify NGC 2146 as a starburst galaxy.
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