Neutron star envelopes and thermal radiation from the magnetic surface

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The thermal structure of neutron star envelopes is discussed with emphasis on analytic results. Recent progress on the effect of chemical constitution and high magnetic fields on the opacities and the thermal structure is further reviewed in view of the application to pulsar cooling and magnetars.
22 pages, 3 figures; LaTeX2e using crckapb.sty (included) and epsf.sty. Invited review at the NATO ASI "The Neutron Star - Black Hole Connection" (Elounda, Crete, 7-18 June 1999), eds. C. Kouveliotou, J. van Paradijs, J. Ventura (Kluwer, to be published)

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