Probabilistic orbits and dynamical masses of emission-line binaries

The observed orbits of emission-line stars may be affected by systematics owing to their broad emission lines being formed in complex and extended environments. This is problematic when orbital parameter probability distributions are estimated assuming radial-velocity data are solely comprised of Ke...

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Bibliographic Details
Main Authors: Grant, D, Blundell, K
Format: Journal article
Language:English
Published: Royal Astronomical Society 2021