canonical IMF IMF-e hanjârvâr Fr.: IMF canonique A two-component stellar → initial mass function with → slopes of 1.3 and 2.3 for massive and low mass stars, respectively. Also called universal IMF. |
top-heavy IMF IMF-e bâlâ-sangin Fr.: A star formation process in which → massive stars form more abundantly than that predicted by standard models, whereby the top end of the → initial mass function is significantly flatter than the canonical → Salpeter slope. → top; → heavy; → initial mass function. |
universal IMF IMF-e hargâni Fr.: IMF universelle Same as → canonical IMF. |