Featured Image: Tracking Motions of Local Galaxies
Abstract
Whats with all the dots? Youre looking at the positions of thousands of stars observed by the Gaia mission in and around two nearby galaxies: Andromeda (M31) and Triangulum (M33). In a new study led by Roeland van der Marel (Space Telescope Science Institute and Johns Hopkins University), a team of scientists used stellar proper-motion observations from Gaias second data release, DR2, to track the 3D movement of these two galaxies. The precision of the Gaia data allowed the authors to update our best estimates about how these galaxies are interacting with each other and with the Milky Way, both now and in the future. Van der Marel and collaborators find that the Triangulum galaxy is likely on its very first infall into Andromeda, suggesting its not to blame for Andromedas previously formed tidal warps and tails. And Andromeda itself appears to be on a less direct path toward us than wed previously thought, suggesting the collision between Andromeda and the Milky Way may be only glancing, and it wont occur for another 4.5 billion years. For more on the authors conclusions, check out the article below.CitationFirst Gaia Dynamics of the Andromeda System: DR2 Proper Motions, Orbits, and Rotation of M31 and M33, Roeland P. van der Marel et al 2019 ApJ 872 24. doi:10.3847/1538-4357/ab001b
- Publication:
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AAS Nova Highlights
- Pub Date:
- February 2019
- Bibcode:
- 2019nova.pres.4791K
- Keywords:
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- Highlights;
- Images;
- galaxies;
- galaxy interactions;
- galaxy kinematics;
- Local Group