A New Method for the Determination of the Hubble Parameter

By chance, the slope of the Mv(max) versus (B-V)max relation for recenttheoretical models of supernovae of Type Ia (SNe Ia) by Hoflich & Khokhlov isindistinguishable from the slope of a reddening line in the V versus B-V plane.This coincidence allows one to determine a parameter Mv*(max) for SNe Ia thatis independent of both supernova detonation model and of interstellarreddening. Calibrating Mv*(max) with observations of SNe Ia by Hamuy et al.yields values of the Hubble parameter Ho in the range 55 - 60 km s-1 Mpc-1 .The discrepancy between this result, and values of Ho recently obtained fromobservations of Cepheids in the Virgo cluster, suggests that either (1) theCepheid distance scale is wrong, (2) the SN Ia models of Hoflich & Khokhlov aretoo bright by ~ 0.75 mag near maximum light, or (3) their models are too red by\~ 0.25 mag in B-V.