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Autor:
Dmytrenko, A. M., Fedorov, P. N., Akhmetov, V. S., Velichko, A. B., Denyshchenko, S. I., Khramtsov, V. P., Vavilova, I. B., Dobrycheva, D. V., Sergijenko, O. M., Vasylenko, A. A., Kompaniiets, O. V.
We present the results of determining the parameters characterizing the shape and orientation of residual velocity ellipsoids from the Gaia DR3 red giants and subgiants. We show the distribution of velocity dispersions in the Galactic plane obtained
Externí odkaz:
http://arxiv.org/abs/2412.18333
