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Gaia's view of the Milky Way's neighbouring galaxies

Gaia's view of the Milky Way's neighbouring galaxies


Date: 03 December 2020
Satellite: Gaia
Copyright: ESA/Gaia/DPAC; CC BY-SA 3.0 IGO. Acknowledgement: L. Chemin; X. Luri et al (2020)

The Large and Small Magellanic Clouds (LMC and SMC, respectively) are two dwarf galaxies that orbit the Milky Way. This image shows the stellar density of the satellite galaxies as seen by Gaia in its Early Data Release 3, which was made public on 3 December 2020. It is composed of red, green and blue layers, which trace mostly the older, intermediate age, and younger stars respectively.

Astronomers place stars into categories that are often named for their colour and appearance.

In this image, the red layer contains evolved stars that compose the Red Giant Branch and Red Clump stars. The green layer contains Main Sequence stars of mixed ages of up to two billion years. The blue layer contains stars younger than 400 million years, Asymptotic Giant Branch stars, and RR-Lyrae and classical Cepheid variable stars.

The brightnesses used in this image are based on a logarithmic scale to enhance low surface density regions in the galaxies, for example the outer spiral arm in the LMC visible in the upper left.

The density of younger stars has been artificially enhanced with respect to the other evolutionary phases to make them more clearly visible. This shows that younger stars mostly trace the inner spiral structure of the LMC, and the 'bridge' of stars between the two galaxies. Finally, intermediate age and older stars trace the LMC bar, spiral arms, and outer halo, as well as the SMC outer halo.

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This work is licensed under a Creative Commons Attribution-ShareAlike 3.0 IGO License. Creative Commons License

Last Update: 9 December 2020
24-Sep-2021 11:21 UT

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