Published August 1976
| Version v1
Journal article
Radiative transfer in hydrodynamical protostar models I
Description
A method of solution of the non-grey radiative transfer problem in the extended envelopes of protostars is described. This method has been coupled to the hydrodynamical evolutionary code of Appenzeller and Tscharnuter (1974, 1975). Preliminary numerical results for the evolution in spectral appearance of a 1M(S) protostar are discussed. (orig.)
Abstract (German)
Es wird eine Methode zur Loesung des nicht grauen Strahlungstransportproblems in ausgedehnten Huellen von Protosternen beschrieben. Diese Methode wurde in das Programm der hydrodynamischen Entwicklung von Appenzeller und Tscharnuter (1974, 1975) eingefuegt. Vorlaeufige nummerische Ergebnisse der Entwicklung der spektralen Erscheinung eines Protosterns mit 1M(S) werden diskutiert. (orig.)Additional details
Additional titles
- Subtitle (English)
- Method and preliminary results
Publishing Information
- Journal Title
- Astron. Astrophys.
- Journal Volume
- 51
- Journal Issue
- 1
- Series
- Astron. Astrophys.
- Journal Page Range
- 101-105
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- Germany
- INIS RN
- 8300425
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- HYDRODYNAMIC MODEL; HYDRODYNAMICS; NUMERICAL SOLUTION; PROTOSTARS; RADIATION TRANSPORT; TEMPERATURE DEPENDENCE; TRANSPORT THEORY
- Descriptors DEC
- FLUID MECHANICS; MATHEMATICAL MODELS; MECHANICS; PARTICLE MODELS; STATISTICAL MODELS; THERMODYNAMIC MODEL
Optional Information
- Notes
- 5 figs.; with refs.