Stellar Content of the Galactic Starburst Template NGC 3603 from Adaptive Optics Observations*

, , , and

© 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation F. Eisenhauer et al 1998 ApJ 498 278 DOI 10.1086/305552

0004-637X/498/1/278

Abstract

We present near-infrared adaptive optics imaging of the Galactic starburst template NGC 3603 and its stellar center HD 97950. There is clear evidence for the presence of stars down to 1 Script M or less. No cutoff or turnover in the initial mass function is evident. Applying theoretical models of the pre-main-sequence evolution of intermediate-mass stars to the observed color-color diagram, the color-magnitude diagram, and the luminosity function, we constrain both the age distribution and the initial mass function. Within the systematic errors, this initial mass function follows a Salpeter power law with index Γ ≤ -0.73 down to the observational limit of less than 1 Script M. The stars with less than 4 Script M appear to be younger than 106 yr, in contrast to previous age determinations of the high-mass content of HD 97950.

Export citation and abstract BibTeX RIS

Footnotes

  • Based on observations collected at the European Southern Observatory, La Silla, Chile, ESO 54.E-1000, ESO 56.D-0573, ESO 57.D-0354.

Please wait… references are loading.
10.1086/305552