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Extended Atmospheres of Planetary Nuclei
Published online by Cambridge University Press: 08 February 2017
Abstract
Exploratory calculations on nongray, hydrostatic-equilibrium model envelopes for central stars of planetary nebulae of high temperature and possibly near the instability limit are reported. It is conjectured that these may be related to Wolf-Rayet type nuclei; it appears possible to obtain an OV absorption, and OVI emission, spectrum even in an LTE calculation.
- Type
- Part A. Type of Problems that Exist
- Information
- International Astronomical Union Colloquium , Volume 2: Spectrum Formation in Stars With Steady-State Extended Atmospheres , August 1970 , pp. 54 - 60
- Copyright
- Copyright © 1970