Celestial hemisphere:  Northern  ·  Constellation: Leo (Leo)  ·  Contains:  IC 2708  ·  IC 2745  ·  Leo Triplet  ·  M 65  ·  M 66  ·  NGC 3623  ·  NGC 3627  ·  NGC 3628
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Leo Triplet (M 65, M 66, NGC 3628), Alex Woronow
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Leo Triplet (M 65, M 66, NGC 3628)

Getting plate-solving status, please wait...
Leo Triplet (M 65, M 66, NGC 3628), Alex Woronow
Powered byPixInsight

Leo Triplet (M 65, M 66, NGC 3628)

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Description

OTA: Star-Fire 175 (f/8)

Camera: FLI - PL16070AE

Observatory: Deep Sky West

EXPOSURES:

Red: 24 x 900 seconds

Blue: 14 x 900

Green: 26 x 900

Lum.: 32 x 900

Total exposure 24 hours

Image Width: ~1.5 deg

Processed by Alex Woronow using PixInsight & StarNet++ in 2019

The “Leo Triplet” consists of the three spiral galaxies listed in the title. They lie about 35M light-years from us. These galaxies are mutually interacting, gravitationally, which likely accounts for the streamer of gas, dust, and/or stars trailing downward in this picture from the left-most galaxy, NGC 3628. NGC 3628 also exhibits obvious distortions from the archetypical lenticular profile of spiral galaxies, being flared at its extremities. Our edge-on view of NGC 3628 also shows a complexly structured medial band of dust and gas obscuring the stars in the plane of the galaxy. M 66 (left-most galaxy) shows a weak barred structure and has an unusually high proportion of its mass concentrated at its center. You should be able to see a faint bulge of material to its left--probably due to its gravitational interaction with NGC 3628. Finally, M 65 is poor in gas and dust (having been stripped in gravitational encounters, I expect) and consequently has little active star-formation (and a dearth of blue stars.)

(Source: largely Wikipedia)

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Leo Triplet (M 65, M 66, NGC 3628), Alex Woronow

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