The Impact of Feedback in Massive Star Formation. II. Lower Star Formation Efficiency at Lower Metallicity
Journal article, 2018

We conduct a theoretical study of the formation of massive stars over a wide range of metallicities from 10-5to and evaluate the star formation efficiencies (SFEs) from prestellar cloud cores taking into account multiple feedback processes. Unlike for simple spherical accretion, feedback processes in the case of disk accretion do not set upper limits on stellar masses. At solar metallicity, launching of magneto-centrifugally driven outflows is the dominant feedback process to set SFEs, while radiation pressure, which has been regarded as pivotal, makes only a minor contribution even in the formation of stars over 100 M⊙. Photoevaporation becomes significant in the formation of stars over 20 M⊙at low metallicities of ≲ 10-2Z⊙, where dust absorption of ionizing photons is inefficient. We conclude that if initial prestellar core properties are similar, then massive stars are rarer in extremely metal-poor environments of 10-5-10-3Z⊙. Our results give new insight into the high-mass end of the initial mass function and its potential variation with galactic and cosmological environments.

stars: formation

outflows

stars: evolution

stars: luminosity function

mass function

stars: massive

stars: winds

Author

Kei E.I. Tanaka

University of Florida

National Astronomical Observatory of Japan

Osaka University

Jonathan Tan

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics, Galactic Astrophysics

University of Virginia

Yichen Zhang

RIKEN

Takashi Hosokawa

Kyoto University

Astrophysical Journal

0004-637X (ISSN) 1538-4357 (eISSN)

Vol. 861 1 68

Subject Categories

Astronomy, Astrophysics and Cosmology

Atom and Molecular Physics and Optics

Other Physics Topics

DOI

10.3847/1538-4357/aac892

More information

Latest update

3/29/2021