Explore: Initial Mass Function

In astronomy, the initial mass function (IMF) is an empirical function that describes the initial distribution of masses for a population of stars during

production in stars. He later derived the initial mass function for the formation rates of stars of different mass in the Galaxy. Salpeter wrote with Hans

binary system Halo mass function, a function that describes the mass distribution of dark matter halos Initial mass function, a function that describes the

star, must also account for the statistics of binary stars and the initial mass function. Most stars do not form in isolation but as part of a group of stars

fluid dynamics, the Iribarren parameter. The initial mass function in astronomy. The correlation function in astronomy. Spatial frequency; also sometimes

of newly formed stars is described empirically by the initial mass function.) During the initial collapse, this pre-main-sequence star generates energy

body mass), and the social sciences (e.g. city sizes and income). Among them are: Neural scaling law Kepler's third law The initial mass function of stars

of plasma cells in the bone marrow Inframammary fold, in anatomy Initial mass function, in stellar astronomy Intermolecular force, non-bonding electrostatic

observe the same distribution of stellar masses—the initial mass function—apparently regardless of the initial conditions? Supernova: What is the mechanism by

6505 were estimated. One result is that the central region has an initial mass function that is heavier than predicted with Chabrier and a dark matter fraction