Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-10-18
Mon.Not.Roy.Astron.Soc.Lett. 374 (2007) L29-L33
Astronomy and Astrophysics
Astrophysics
5 pages including 3 figures; accepted for publication in MNRAS
Scientific paper
10.1111/j.1745-3933.2006.00258.x
Understanding the origin of stellar masses is a key problem in astrophysics. In the solar neighborhood, 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 circum-nuclear starburst regions. The resulting IMF is top-heavy with a peak at ~ 15 Msun, a sharp turn-down below 7 Msun 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 occuring at a temperature of ~ 100 K and an H2 density of a few times 10^5 cm^-3, and discuss possible implications for galaxy formation and evolution.
Jappsen Anne-Katharina
Klessen Ralf S.
Spaans Marco
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