We study neutrino-photon processes such as gamma gamma-->nu<(<nu>)over bar>
in the presence of a uniform external magnetic field for the case when neu
trinos can couple to the electromagnetic field directly through their dipol
e magnetic moment and obtain the stellar energy loss. The process would be
of special relevance in astrophysical situations where standard left-handed
neutrinos are trapped and the right-handed neutrinos produced through the
spin Aip interaction induced by the neutrino magnetic moment alone can free
ly stream out.