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The Dynamics of Interstellar Asteroids and Comets within the Galaxy: An Assessment of Local Candidate Source Regions for 1I/'Oumuamua and 2I/Borisov

Tim Hallatt, Paul Wiegert, 2020. The Astronomical Journal.

Shows that scattering by the Galactic disc limits any back-integration to about 15 pc accuracy at 10 million years and 400 pc at 100 million, so a home star can only be named statistically; finds the origin likely within 1 kpc and the Carina and Columba moving groups the most plausible source regions. AJ 159, 147.

MYS0CSKBPVW6FBV · mystery · click to copyM1I/'OumuamuaArticledoi: 10.3847/1538-3881/ab7336Checked against the original0

What it's used for here

Why the traceback cannot name a single home star.

Cited by on this site 4 records

Cite it

Hallatt, T., & Wiegert, P. (2020). The Dynamics of Interstellar Asteroids and Comets within the Galaxy: An Assessment of Local Candidate Source Regions for 1I/'Oumuamua and 2I/Borisov. The Astronomical Journal. https://doi.org/10.3847/1538-3881/ab7336
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