Celestial hemisphere:  Northern  ·  Constellation: Leo Minor (LMi)  ·  Contains:  HD94087  ·  HD94178  ·  IC 2608  ·  NGC 3395  ·  NGC 3396  ·  NGC 3413  ·  NGC 3424  ·  NGC 3430  ·  PGC 2011371  ·  PGC 2014189  ·  PGC 2014899  ·  PGC 2015795  ·  PGC 2017489  ·  PGC 2021619  ·  PGC 32631  ·  PGC 32658
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Arp270 and Leo Minor Galaxy Cluster in LRGB, David Payne
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Arp270 and Leo Minor Galaxy Cluster in LRGB

Getting plate-solving status, please wait...
Arp270 and Leo Minor Galaxy Cluster in LRGB, David Payne
Powered byPixInsight

Arp270 and Leo Minor Galaxy Cluster in LRGB

Equipment

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Acquisition details

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Description

Leo Minor Galaxy Cluster in LRGB, March 2023
Planewave CDK12.5" telecope and A-P 1100GTO AE mount
ASI6200MM, Antlia Pro BB & 3nm Ha Filters
Lum (28 x 180s exposures, Bin 2x2, Gain 100)
RGB (3 x 15 x 180s exposures, Bin 2x2 Gain 100)
Total Integration Time = 3.7 hours

This Galaxy Cluster in Leo Minor seemed a very interesting target as it contains a rich field as well as a member of the ARP catalogue of unusual galaxies.
ARP270, or NGC3395/3396, lie on the left hand side of the frame and actually consists of two interacting/merging galaxies, both of which are undergoing intense star forming activity as a result of the tidal interaction.
The largest galaxy in the field of view is the more stable spiral NGC3430. Nearby is the "Hamburger" shaped NGC3424. These and the next smallest CI2608 nearby are called a "cluster" but, but actually range from 26 to 72 million lys apart. By that measure, the Milky Way might be considered part of the same "cluster" when viewed from an different point.
For this image, I actually changed up my processing path, deciding to do more intense noise reduction at the linear stage rather than at the end. I think I like the result.

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