High Resolution Spectroscopy of White Dwarfs

Details High Resolution Spectroscopy of White Dwarfs High Resolution Spectroscopy of White Dwarfs

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..233m&link_type=abstract

Chandra Proposal ID #01200142

Physics

Chandra Proposal Id #01200142

Scientific paper

H1504+65 is the hottest white dwarf star known. Its atmosphere appears to be devoid of H or He, perhaps from mass loss during several cycles through the red giant phase. If so this star reveals directly the products of nuclear burning in the core of its progenitor. A high resolution spectrum can identify the elements in the photosphere. If present, the detection of Ne and its abundance will provide important information on the physical conditions in the core.

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