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Autor:
Arpit Arora, Robyn E. Sanderson, Sukanya Chakrabarti, Andrew Wetzel, Thomas Donlon II, Danny Horta, Sarah R. Loebman, Lina Necib, Micah Oeur
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 2, p 223 (2024)
Measurements of the accelerations of stars enabled by time-series extreme-precision spectroscopic observations, pulsar timing, and eclipsing binary stars in the solar neighborhood offer insights into the mass distribution of the Milky Way that do not
Externí odkaz:
https://doaj.org/article/50d9b2217a61415a9e93c8f50faca477
