The Contribution of the Absorption Processes to the Opacity of DB White Dwarf Atmospheres in UV and VUV Regions

Details The Contribution of the Absorption Processes to the Opacity of DB White Dwarf Atmospheres in UV and VUV Regions The Contribution of the Absorption Processes to the Opacity of DB White Dwarf Atmospheres in UV and VUV Regions

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1203..121i&link_type=abstract

ORGANIZED BY THE HELLENIC PHYSICAL SOCIETY WITH THE COOPERATION OF THE PHYSICS DEPARTMENTS OF GREEK UNIVERSITIES: 7th Internatio

Physics

Photodissociation, Absorption, White Dwarfs, Photoionisation, Processes Caused By Visible And Uv Light, Electromagnetic Wave Propagation, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Photoionization Of Atoms And Ions

Scientific paper

The main aim of this work is to estimate the total contribution to the opacity of DB white dwarf atmosphere of the processes of the He2+ molecular ion photo-dissociation and He+He+ collisional absorption charge exchange, and compare it with the contribution of He-, and other relevant, radiative absorption processes included in standard models.

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