A multiple power-law distribution for initial mass functions. Issue 2 (11th April 2020)

• Record Type: Journal Article
• Authors: Essex, Christopher; Basu, Shantanu; Prehl, Janett; Hoffmann, Karl Heinz
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 494:Issue 2(2020)
• Page Start: 1579
• Page End: 1586
• Publication Date: 2020-04-11
• Subjects: accretion, accretion discs -- stars: formation; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/staa755
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We introduce a new multi-power-law distribution for the initial mass function (IMF) to explore its potential properties. It follows on prior work that introduced mechanisms accounting for mass accretion in star formation, developed within the framework of general evolution equations for the mass distribution of accreting and non-accreting (proto)stars. This paper uses the same fundamental framework to demonstrate that the interplay between a mass-dependent and a time-dependent step-like dropout rate from accretion leads to IMFs that exhibit multiple power laws for an exponential mass growth. While the mass-dependent accretion and its dropout is intrinsic to each star, the time-dependent dropout might be tied to a specific history such as the rapid consumption of nebular material by nearby stars or the sweeping away of some material by shock waves. The time-dependent dropout folded into the mass-dependent process of star formation is shown to have a significant influence on the IMFs.