Abstract
We develop a new star formation (SF) law based on the density PDF of turbulence and on the multi-freefall concept of gas collapse. We derive a relation where the star formation rate (SFR) correlates with the molecular gas mass per multi-freefall time, whereas previous models had used the average, single-freefall time. We define a new quantity called maximum (multi-freefall) gas consumption rate (MGCR) and show that the actual SFR is only about 0.4% of this maximum possible SFR, confirming the observed low efficiency of star formation.
Original language | English |
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Pages (from-to) | 740 |
Number of pages | 1 |
Journal | Proceedings of the International Astronomical Union |
Volume | 11 |
Issue number | A29B |
DOIs | |
Publication status | Published - 2015 |