Spectrophotometry of Cool White Dwarfs

Details Spectrophotometry of Cool White Dwarfs Spectrophotometry of Cool White Dwarfs

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1050a&link_type=abstract

HST Proposal ID #1050

Physics

Hst Proposal Id #1050

Scientific paper

Ultraviolet spectrophotometry will be used to determine whether the ultraviolet blanketing of the coolest DA, DC and DK degenerate stars differ due to the presence of molecular hydrogen and/or heavy metallic elements and/or carbon and whether the coolest DC-DK stars have hydrogen-rich atmospheres. The second question may hold implications for the apparent "cut-off" in the white dwarf luminosity function at Log L/L(sun) = -4, the disk star formation history and age.

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