Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-05T02:09:46.321Z Has data issue: false hasContentIssue false

Hubble Space Telescope observations of Baade's window

Published online by Cambridge University Press:  07 August 2017

W. A. Baum
Affiliation:
Univ. of Washington, Seattle, WA 98195, USA
R. M. Light
Affiliation:
Univ. of California, Santa Cruz, CA 95064, USA
J. Holtzman
Affiliation:
Lowell Obs., Flagstaff, AZ 86001, USA
D. Hunter
Affiliation:
Lowell Obs., Flagstaff, AZ 86001, USA
T. Kreidl
Affiliation:
Lowell Obs., Flagstaff, AZ 86001, USA
E. J. O'Neil Jr.
Affiliation:
Kitt Peak Nat Obs., Tucson, AZ 85726, USA

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

This is a status report on a continuing program using the Hubble Space Telescope (HST) Wide–Field Camera (WFC) to probe the stellar population of the Galactic bulge to fainter magnitudes. We seek the mean age of the stars and the initial mass function (IMF). Galactic bulge stars offer the only opportunity to investigate the IMF of a super metal–rich population. They are 100 times closer than the next nearest sample.

Type
Contributed Papers
Copyright
Copyright © Kluwer 1993 

References

Buonanno, R. 1986. Mem. Soc. Astron. Ital. 57, 333.Google Scholar
Green, E. M., Demarque, P., and King, C. R. 1987. The Revised Yale Isochrones and Luminosity Functions (New Haven: Yale Univ. Observatory).Google Scholar
MacKenty, J. W. 1992. HST Wide–Field/Planetary Camera Instrument Handbook (Baltimore: Space Telescope Science Institute).Google Scholar
Harris, H. C., Baum, W. A., Hunter, D. A., and Kreidl, T. J. 1991. Astron.J. 101, 677.CrossRefGoogle Scholar
Lauer, T. R. 1989. Publ. Astron. Soc. Pac. 101, 445.CrossRefGoogle Scholar
Terndrup, D. M. 1988. Astron.J. 96, 884.CrossRefGoogle Scholar
Westphal, J. A. 1982. In The Space Telescope Observatory NASA CP-2244, ed. Hall, D. N. B. (Washington: NASA Scientific and Technical Information Branch), 28.Google Scholar