The Chandra LETGS Soft X-ray Spectrum of the White Dwarf GD153

Physics

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Scientific paper

To calibrate X-ray instruments at low energies high resolution spectra of isolated white dwarfs are needed. So far only only HZ43 and Sirius B have been observed and studied in detail with the Chandra LETGS and EUVE. With this proposed Chandra LETGS observation and the existing EUVE data we will be able to further contrain the physical parameters the white dwarf GD153. Like this with the help of the three independant physical models for these white dwarfs we will be able to better calibrate low energy response (E<0.2keV) of existing and future X-ray detectors.

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