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Hubble inspects a contorted spiral galaxy

by Staff Writers Munich, Germany (SPX) May 28, 2021 SPX
This striking image showcases the unusually contorted appearance of NGC 2276, an appearance caused by two different astrophysical interactions - one with the superheated gas pervading galaxy clusters, and one with a nearby galactic neighbour.

The interaction of NGC 2276 with the intracluster medium - the superheated gas lying between the galaxies in galaxy clusters - has ignited a burst of star formation along one edge of the galaxy.

This wave of star formation is visible as the bright, blue-tinged glow of newly formed massive stars towards the left side of this image, and gives the galaxy a strangely lopsided appearance. NGC 2276's recent burst of star formation is also related to the appearance of more exotic inhabitants - black holes and neutron stars in binary systems.

On the other side of the galaxy from this burst of new stars, the gravitational attraction of a smaller companion is pulling the outer edges of NGC 2276 out of shape. This interaction with the small lens-shaped galaxy NGC 2300 has distorted the outermost spiral arms of NGC 2276, giving the false impression that the larger galaxy is orientated face-on to Earth [1].

NGC 2276 and its disruptive companion NGC 2300 can both be seen in the accompanying image, which shows a wider view of the interacting galaxies.

NGC 2276 is by no means the only galaxy with a strange appearance. The Atlas of Peculiar Galaxies - a catalogue of unusual galaxies published in 1966 - contains a menagerie of weird and wonderful galaxies, including spectacular galaxy mergers, ring-shaped galaxies, and other galactic oddities.

As befits an unusually contorted galaxy, NGC 2276 has the distinction of being listed in the Atlas of Peculiar Galaxies twice - once for its lopsided spiral arms and once for its interaction with its smaller neighbour NGC 2300.

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