By means of deep FORS1/VLT and ACS/Hubble Space Telescope observations of a wide area in the stellar system ? Cen we measured the luminosity function of main-sequence stars down to R = 22.6 and IF814W = 24.5. The luminosity functions obtained have been converted into mass functions and compared with analytical initial mass functions (IMFs) available in the literature. The mass function obtained, reaching M ~ 0.15Msolar, can be well reproduced by a broken power law with indices ? = -2.3 for M > 0.5Msolar and ? = -0.8 for M < 0.5Msolar. Since the stellar populations of ? Cen have been proved to be actually unaffected by dynamical evolution processes, the mass function measured in this stellar system should represent the best approximation of the IMF of a star cluster. The comparison with the MF measured in other Galactic globular clusters suggests that possible primordial differences in the slope of the low-mass end of their MF could exist.
The mass function of Omega Centauri down to 0.15 Msolar
SOLLIMA, ANTONIO;FERRARO, FRANCESCO ROSARIO;
2007
Abstract
By means of deep FORS1/VLT and ACS/Hubble Space Telescope observations of a wide area in the stellar system ? Cen we measured the luminosity function of main-sequence stars down to R = 22.6 and IF814W = 24.5. The luminosity functions obtained have been converted into mass functions and compared with analytical initial mass functions (IMFs) available in the literature. The mass function obtained, reaching M ~ 0.15Msolar, can be well reproduced by a broken power law with indices ? = -2.3 for M > 0.5Msolar and ? = -0.8 for M < 0.5Msolar. Since the stellar populations of ? Cen have been proved to be actually unaffected by dynamical evolution processes, the mass function measured in this stellar system should represent the best approximation of the IMF of a star cluster. The comparison with the MF measured in other Galactic globular clusters suggests that possible primordial differences in the slope of the low-mass end of their MF could exist.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.