This means that inflation-produced fields can reach astrophysically relevant residual strengths without breaking away from standard physics.
Christos G. Tsagas 2016, 'On the Magnetic Evolution in Friedmann Universes and the Question of Cosmic Magnetogenesis',Symmetryhttp://www.mdpi.com/2073-8994/8/11/122. Retrieved from DOAJ CC BY 4.0 (https://creativecommons.org/licenses/by-sa/4.0/legalcode)
For the same pairs the total mass was also found astrophysically - by applying the mass-luminosity relation.
Cvetković Zorica, Ninković S. 2010, 'On the component masses of visual binaries', Serbian Astronomical Journalhttp://www.doiserbia.nb.rs/img/doi/1450-698X/2010/1450-698X1080071C.pdf. Retrieved from DOAJ CC BY 4.0 (https://creativecommons.org/licenses/by-sa/4.0/legalcode)