Footprint of the WFPC2 images for
each of the three sets of HST observations
of NGC 4449 shown superposed on a V-band ground-based image.
The ground-based image was obtained for us by P. Massey
using the 4 m telescope at Kitt Peak National Observatory
(Hunter, van Woerden, & Gallagher 1999).
(Funded in part by the Lowell Research Fund and by NSF through grant
AST-9616940 to DAH.
Work by AEG was funded by the NSF through
the Research Experiences for Undergraduates program,
under grant number 9423921 to Northern Arizona University.)
A false-color combination of three images of the irregular galaxy NGC 4449.
F814W (=I) is shown in red, F555W (=V) is in green, and F336W (=U) is blue.
This is position 1 in the previous image.
(Funded in part by the Lowell Research Fund and by NSF through grant
AST-9616940 to DAH.
Work by AEG was funded by the NSF through
the Research Experiences for Undergraduates program,
under grant number 9423921 to Northern Arizona University.)
A false-color combination of three images of the irregular galaxy NGC 4449.
F814W (=I) is shown in red, F555W (=V) is in green, and F336W (=U) is blue.
This is position 2 in the previous image.
(Funded in part by the Lowell Research Fund and by NSF through grant
AST-9616940 to DAH.
Work by AEG was funded by the NSF through
the Research Experiences for Undergraduates program,
under grant number 9423921 to Northern Arizona University.)
A false-color combination of three images of the irregular galaxy NGC 4449.
F814W (=I) is shown in red, F555W (=V) is in green, and F336W (=U) is blue.
This is position 1 in the previous image.
(Funded in part by the Lowell Research Fund and by NSF through grant
AST-9616940 to DAH.
Work by AEG was funded by the NSF through
the Research Experiences for Undergraduates program,
under grant number 9423921 to Northern Arizona University.)
A false-color combination of three images of the irregular galaxy NGC 4449.
F814W (=I) is shown in red, F555W (=V) is in green, and F336W (=U) is blue.
This is position 2 in the previous image.
(Funded in part by the Lowell Research Fund and by NSF through grant
AST-9616940 to DAH.
Work by AEG was funded by the NSF through
the Research Experiences for Undergraduates program,
under grant number 9423921 to Northern Arizona University.)