HST Observations of Hot DQ White Dwarfs

Details HST Observations of Hot DQ White Dwarfs HST Observations of Hot DQ White Dwarfs

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273...64d&link_type=abstract

17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 64-69 (2010).

Physics

2

White Dwarfs, Spectroscopy, Magnetic Fields, Stellar Evolution, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Spectroscopy And Spectrophotometry, Interplanetary Magnetic Fields, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

We present a preliminary analysis of the recently discovered
carbon-dominated atmosphere white dwarfs (``Hot DQ'') based on HST/COS
observations. We also present a summary of the recent findings that
emerged from our ongoing campaign aimed at obtaining high
signal-to-noise optical spectroscopic observations of these objects.

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