Physics
Scientific paper
Dec 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.8059c&link_type=abstract
HST Proposal ID #8059
Physics
Hst Proposal Id #8059
Scientific paper
The parallel opportunities available with WFPC2 in the neighborhood of bright galaxies are treated in a slightly different way from the normal pure parallels. Local Group galaxies offer the opportunity for a closer look at young stellar populations. Narrow-band images in F656N can be used both to identify young stars via their emission lines, and to map the gas distribution in star-forming regions. Thus, the filter F656N is added to the four standard filters. Near more distant galaxies, up to about 10 Mpc, we can map the population of globular clusters; for this purpose, F300W is less useful, and only F450W, F606W, and F814W will be used.
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