When Galaxies Collide: Hubble Showcases 6 Magnificent Galaxy Mergers

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To celebrate a new year, the NASA/ESA Hubble Space Telescope has published a montage of six beautiful galaxy mergers.

Each of these merging systems was studied as part of the recent HiPEEC survey to investigate the rate of new star formation within such systems.

These interactions are a key aspect of galaxy evolution and are among the most spectacular events in the lifetime of a galaxy.

It is during rare merging events that galaxies undergo dramatic changes in their appearance and in their stellar content.

These systems are excellent laboratories to trace the formation of star clusters under extreme physical conditions.

The Milky Way typically forms star clusters with masses that are 10 thousand times the mass of our Sun.

This doesn’t compare to the masses of the star clusters forming in colliding galaxies, which can reach millions of times the mass of our Sun.

These dense stellar systems are also very luminous.

Even after the collision, when the resulting galactic system begins to fade into a more quiescent phase, these very massive star clusters will shine throughout their host galaxy, as long-lasting witnesses of past merging events.

By studying the six galaxy mergers shown here, the Hubble imaging Probe of Extreme Environments and Clusters (HiPEEC) survey has investigated how star clusters are affected during collisions by the rapid changes that drastically increase the rate at which new stars are formed in these galaxies.

Hubble’s capabilities have made it possible to resolve large star-forming “knots” into numerous compact young star clusters. Hubble’s ultraviolet and near-infrared observations of these systems have been used to derive star cluster ages, masses, and extinctions and to analyze the star formation rate within these six merging galaxies.

The HiPEEC study reveals that the star cluster populations undergo large and rapid variations in their properties, with the most massive clusters formed towards the end of the merger phase.

Each of the merging systems shown here has been previously published by Hubble, as early as 2008 and as recently as October 2020.

To celebrate its 18th anniversary in 2008, the Hubble Space Telescope released a collection of 59 images of merging galaxies, which can be explored here.

More information
Reference: “Star cluster formation in the most extreme environments: insights from the HiPEEC survey” by A Adamo, K Hollyhead, M Messa, J E Ryon, V Bajaj, A Runnholm, S Aalto, D Calzetti, J S Gallagher, M J Hayes, J M D Kruijssen, S König, S S Larsen, J Melinder, E Sabbi, L J Smith and G Östlin, 3 September 2020, Monthly Notices of the Royal Astronomical Society.DOI: 10.1093/mnras/staa2380
The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

The HiPEEC survey was completed as part of the Hubble Space Telescope program GO 14066 (PI: A.

Adamo).

A repository with the study’s final data and catalogs is available here in the MAST Archive.

The international team of astronomers in this study consists of A.

Adamo, K. Hollyhead, M. Messa, J.

E. Ryon, V.

Bajaj, A. Runholm, A.

Aalto, D.

Calzeti, J. S. Gallagher, M. J. Hayes, J. M.

D. Kruijssen, S. König, S. S. Larsen, J. Melinder, E. Sabbi, L. J. Smith, and G. Östlin.

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