A young spectroscopic binary in a quintuple system part of the Local Association
Context. Double-lined spectroscopic (SB2) binaries allow us to obtain a direct determination of the masses of their components, which is essential to test stellar models. Although these objects only provide a lower limit for the mass, they are more abundant than their eclipsing counterparts as they are not as strongly limited by the inclination of
Cardona Guillén, Carlos et al.
Advertised on:
10
2021