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Lyman Gamma Satellites Due to H-H+ Collisions: Application to FUSE Observations of Hot White Dwarfs

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White Dwarfs

Part of the book series: NATO Science Series ((NAII,volume 105))

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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

  • Print ISBN: 978-1-4020-1364-5

  • Online ISBN: 978-94-010-0215-8

  • eBook Packages: Springer Book Archive

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