Studies of Blue Compact Dwarf Galaxies

Details Studies of Blue Compact Dwarf Galaxies Studies of Blue Compact Dwarf Galaxies

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1246d&link_type=abstract

HST Proposal ID #1246

Computer Science

Hst Proposal Id #1246

Scientific paper

It is proposed to observe a few blue compact dwarf galaxies at high angular resolution. The most massive stars are expected to be resolved and identified by an exposure through a far UV filter. Further exposures with a near UV and visible filters would give their colors. The aim is to determine how star formation may be affected by the extreme conditions known to be present in this category of objects (intense burst of star formation, low heavy element abundances, large amount of neutral hydrogen). An exposure with the WF/PC in the far red is supposed to reveal the possible existence of an older generation of stars.

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