2006/10/18 by Ralf S. Klessen, Marco Spaans, Anne‐Katharina Jappsen +1 · 1 citation
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Galaxy #Initial mass function #Milky Way #Physics #Solar mass #Star formation #Stars #Stellar mass #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1111/j.1745-3933.2006.00258.x
published as Mon.Not.Roy.Astron.Soc.Lett. 374 (2007) L29-L33 · 5 pages including 3 figures; accepted for publication in MNRAS
arxiv created 2006/10/18 · openalex publication_date 2006/11/14 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Abstract Understanding the origin of stellar masses is a key problem in astrophysics. In the solar neighbourhood, the mass distribution of stars follows a seemingly universal pattern. In the centre of the Milky Way, however, there are indications for strong deviations and the same may be true for the nuclei of distant starburst galaxies. Here we present the first numerical hydrodynamical calculations of stars formed in a molecular region with chemical and thermodynamic properties similar to those of warm and dusty circumnuclear starburst regions. The resulting initial mass function is top-heavy with a peak at ∼15 M⊙, a sharp turn-down below ∼7 M⊙ and a power-law decline at high masses. We find a natural explanation for our results in terms of the temperature dependence of the Jeans mass, with collapse occurring at a temperature of ∼100 K and an H2 density of a few ×105 cm−3, and discuss possible implications for galaxy formation and evolution.