The Temperature of the Hot DB GD 190
DOI: 10.1515/astro-2000-0110
Bibcode: 2000BaltA...9...43P
Provencal, J. L.; Shipman, H. L.
United States
Abstract
We are currently in the midst of an investigation of hydrogen and carbon abundances in hot DB white dwarfs. Our HST UV spectra give evidence that hot DBs contain traces of carbon which can be used to determine the temperatures of these objects. We present the results of our investigation of GD 190.
2000
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Baltic Astronomy
eHST
0