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Backwarming Effect of Molecular Opacities on the Infrared Colours of Very Cool White Dwarfs

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Dust and Molecules in Evolved Stars

Abstract

Recent observations of intrinsically faint objects have increased the num­ber of very cool white dwarfs. Photometry as well as spectroscopy by Ruiz et al. (1992, 1997) and Bergeron et al. (1997) revealed a variety of spec­tral shapes ranging from pure continuum to broadened and shifted features of hydrogen, neutral helium or of carbon bands if their identification was possible. Some objects show strange depressions of infrared colours which could not be accurately reproduced by hotter model atmospheres and qua­sicontinuous spectra.

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© 1997 Springer Science+Business Media Dordrecht

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Bues, I., Aslan, T. (1997). Backwarming Effect of Molecular Opacities on the Infrared Colours of Very Cool White Dwarfs. In: Cherchneff, I., Millar, T.J. (eds) Dust and Molecules in Evolved Stars. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1307-8_23

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  • DOI: https://doi.org/10.1007/978-94-017-1307-8_23

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5018-2

  • Online ISBN: 978-94-017-1307-8

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