Balman, S. 1998. Application of the hot white dwarf atmosphere models to the X-ray data of classical novae. Conference of the NATO-Advanced-Study-Institute on Variable Stars as Essential Astrophysical Tools , (CESME, Turkey), 773-782.

Balman, S., (1998). Application of the hot white dwarf atmosphere models to the X-ray data of classical novae . Conference of the NATO-Advanced-Study-Institute on Variable Stars as Essential Astrophysical Tools (pp.773-782). CESME, Turkey

Balman, ŞÖLEN. "Application of the hot white dwarf atmosphere models to the X-ray data of classical novae," Conference of the NATO-Advanced-Study-Institute on Variable Stars as Essential Astrophysical Tools, CESME, Turkey, 1998

Balman, ŞÖLEN. "Application of the hot white dwarf atmosphere models to the X-ray data of classical novae." Conference of the NATO-Advanced-Study-Institute on Variable Stars as Essential Astrophysical Tools , CESME, Turkey, pp.773-782, 1998

Balman, S. (1998) . "Application of the hot white dwarf atmosphere models to the X-ray data of classical novae." Conference of the NATO-Advanced-Study-Institute on Variable Stars as Essential Astrophysical Tools , CESME, Turkey, pp.773-782.

@conferencepaper{conferencepaper, author={ŞÖLEN BALMAN}, title={Application of the hot white dwarf atmosphere models to the X-ray data of classical novae}, congress name={Conference of the NATO-Advanced-Study-Institute on Variable Stars as Essential Astrophysical Tools}, city={CESME}, country={Turkey}, year={1998}, pages={773-782} }