This parameter decreases very rapidly in Wolf-Rayet stars.
The initial distribution of this quantity, which can be estimated from current values using the method of Miller and Scalo, varies according to a power law with an exponent of -2.35 according to the Salpeter formula. This quantity and chemical composition uniquely determine all other properties according to the Vogt-Russell theorem. Donald Figer proposed a maximum attainable value for this quantity by studying the Arches Cluster. This quantity is raised to a power of roughly 3.5 to compute (*) luminosity for main-sequence stars. This parameter decreases very rapidly in Wolf-Rayet stars. White dwarfs which exceed the sun in this measure by a factor of 1.4 will collapse to neutron stars according to the Chandrasekhar limit. For 10 points, name this stellar parameter, which is often measured relative to the Sun's value of roughly 10^30 kilograms.
The initial distribution of this quantity, which can be estimated from current values using the method of Miller and Scalo, varies according to a power law with an exponent of -2.35 according to the Salpeter formula.
stellar mass