Molecular gas in the host galaxy of the Lensed quasar 0957+561 (QSO 0957+56
1) at the redshift of 1.41 has been detected in the carbon monoxide (CO) Li
ne. This detection shows the extended nature of the molecular gas distribut
ion in the host galaxy and the pronounced lensing effects due to the differ
entially magnified CO Luminosity at different velocities. The estimated mas
s of molecular gas is about 4 x 10(9) solar masses, a molecular gas mass ty
pical of a spiral galaxy Like the Milky Way. A second, weaker component of
CO is interpreted as arising from a close companion galaxy that is rich in
molecular gas and has remained undetected so far. Its estimated molecular g
as mass is 1.4 x 10(9) solar masses, and its velocity relative to the main
galaxy is 660 kilometers per second. The ability to probe the molecular gas
distribution and kinematics of galaxies associated with high-redshift Lens
ed quasars can be used to improve the determination of the Hubble constant
H-0.