Abstract
In this poster we present results from applying new machine learning algorithms to stars in Orion. Using new data from Gaia DR3 and SDSS, positions, radial velocities, proper motions, parallaxes, and ages are assembled for available stars in the region. Stars in the sample are clustered into groups based on these characteristics. With current data, we are able to include more details than previous work, which will improve inferences about the past dynamics of stars in Orion.
| Original language | English |
|---|---|
| Article number | 101.07 |
| Journal | Bulletin of the American Astronomical Society |
| Volume | 56 |
| Issue number | 7 |
| DOIs | |
| Publication status | Published - 1 Jul 2024 |
| Event | 244th Meeting of the American Astronomical Society - Monona Terrace Convention Center, Madison, Wisconsin, United States Duration: 9 Jun 2024 → 13 Jun 2025 https://aas.org/meetings/aas244 |
Austrian Fields of Science 2012
- 103003 Astronomy
- 103004 Astrophysics