Celestial hemisphere:  Northern  ·  Constellation: Ursa Major (UMa)  ·  Contains:  NGC 3550  ·  NGC 3552  ·  NGC 3553  ·  NGC 3554  ·  NGC 3558  ·  NGC 3561  ·  PGC 1834590  ·  PGC 1834602  ·  PGC 1835035  ·  PGC 1836391  ·  PGC 1836835  ·  PGC 1836919  ·  PGC 1837035  ·  PGC 1837234  ·  PGC 1837359  ·  PGC 1837891  ·  PGC 1837971  ·  PGC 1838350  ·  PGC 1838667  ·  PGC 1839577  ·  PGC 1839666  ·  PGC 1840109  ·  PGC 1840265  ·  PGC 1840420  ·  PGC 1840471  ·  PGC 1840677  ·  PGC 1840717  ·  PGC 1840966  ·  PGC 1841722  ·  PGC 1842256  ·  And 66 more.
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Arp 105, "The Guitar". NGC 3561 in Abell 1185, Mau_Bard
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Arp 105, "The Guitar". NGC 3561 in Abell 1185

Getting plate-solving status, please wait...
Arp 105, "The Guitar". NGC 3561 in Abell 1185, Mau_Bard
Powered byPixInsight

Arp 105, "The Guitar". NGC 3561 in Abell 1185

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Description

After three months of adverse weather, including strong winds, I had a full night available to image this wonderful galaxy cluster including Arp 105 "the guitar".

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Abell 1185 lies at around 433 million light years from our galaxy, and is moving away from us at a rate of 8700 km/s due to the cosmic expansion.
The cluster contains 82 confirmed member galaxies for which common red shifts have been found.

One of the cluster's brightest and most interesting objects is Arp 105, "the Guitar". The main protagonists in this maelstrom of interacting galaxies are the spiral galaxy (NGC 3561B) and the elliptical (NGC 3561A), along with a handful of tidal dwarf galaxies. The debris of their gravitational dance renders a shape reminiscent of a guitar.
A small tidal dwarf galaxy known as Ambartsumian's Knot is the blueish speck below NGC 3561, and it is believed to be the remnant of the extensive tidal tail pulled out of one of the galaxies.

The interacting galaxies are flinging out tidal arcs, sheets and knots of their constituent stars across hundreds of thousands of light years. Some of these will potentially form distinct gravitationally bound condensations of stars and gas in their own right - becoming tidal dwarf galaxies. It seems likely that the independence of these new systems can only be a temporary state of affairs, given their location in the middle of a cluster.

Near the center of Abell 1185 (just above the middle of our image here) lies NGC 3550, the brightest cluster galaxy. Look closely at it's center you will see that it contains a rare triple nucleus. These nuclei have greatly differing velocities and it seems that this is the result of a relatively recent set of mergers that has yet to settle down and the nuclei merge.

A close look to the image reveals a quantity of galaxy types and ongoing interactions.

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