Thermal Emission from Binary Millisecond Pulsar Stars (MSPs)

Abstract

Pulsar stars divided into two types depending on the periods of rotation, normal
emission Pulsar and Millisecond pulsars (MSPs). In this paper, the effect of the
strong magnetic field on the thermal emission in Millisecond pulsar stars is
concentrated. Also the luminosity spin down (Lsp) are calculated depends on the
periods (P), and Period derivative (
P
) for sample stars which were adopted. The
relation between internal and surface magnetic field is illustrated. The model that
which adopted is Hallo Cone Model (HCM)). The total magnetic dipole radiation
power (heating power Wh) of all super fluid neutrons in MSPs stars is calculated.
For sample stars of MSPs , the value of transition period (Ptr) was determined by
depending on the some properties of pulsar star. The results indicated that heating
power of our model (A) would be larger than the model (B) that's due to the huge
value of the moment of inertia (I). Also the results showed that the maximum
surface luminosity of stars occurs at the values of Magnetic field ≥ 5.5 1012 Gauss.