Hostname: page-component-745bb68f8f-f46jp Total loading time: 0 Render date: 2025-01-13T00:21:01.852Z Has data issue: false hasContentIssue false
  • English
  • Français

Comparison of Different Treatments of the Radiation Transfer in Model Calculations of Planetary Nebulae

Published online by Cambridge University Press:  19 July 2016

G. Bässgen ,
M. Bässgen  and
M. Grewing
G. Bässgen
Affiliation:
Astronomisches Institut Tübingen (FRG)
M. Bässgen
Affiliation:
Astronomisches Institut Tübingen (FRG)
M. Grewing
Affiliation:
Astronomisches Institut Tübingen (FRG)

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A method of Radiation Transfer treatment (Global Shell Model (GSM)) has been developed, different from the On the Spot Approximation (OSA), taking into account all diffuse reemission from radiative recombination of hydrogen and helium in the nebula itself. For optically thick and optically thin nebulae the method automatically reproduces the On the Spot Approximation and the models without any Radiation Transfer, respectively.

Type
II. Nebular Properties
Information
Symposium - International Astronomical Union , Volume 131: Planetary Nebulae , 1989 , pp. 227
Copyright
Copyright © Kluwer 1989