Abstract
New theoretical calculations of Lyman 7 profiles perturbed by protons allow us to identificate a large feature near 995 Å in FUSE observations of hot white dwarfs. This feature is due to quasi-molecular Lyman γ satellites due to H-H+ collisions near 991 and 996 Å.
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© 2003 Springer Science+Business Media Dordrecht
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Allard, N.F. et al. (2003). Lyman Gamma Satellites Due to H-H+ Collisions: Application to FUSE Observations of Hot White Dwarfs. In: de Martino, D., Silvotti, R., Solheim, JE., Kalytis, R. (eds) White Dwarfs. NATO Science Series, vol 105. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0215-8_47
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DOI: https://doi.org/10.1007/978-94-010-0215-8_47
Publisher Name: Springer, Dordrecht
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