The nature of the 10 and 20 micrometer features in circumstellar dust shells
- 1 December 1983
- journal article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 97 (2) , 405-419
- https://doi.org/10.1007/bf00653496
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Observationally-based infrared efficiencies and planck means for circumstellar dust grainsAstrophysics and Space Science, 1983
- A Model of the 10 Micrometer Silicate Feature in the Spectra of BN‐like IR‐Point Sources (Mitteilungen der Universitäts‐Sternwarte zu Jena Nr. 150)Astronomische Nachrichten, 1982
- Laboratory spectra of protosilicates and the interstellar silicate absorption bandsAstrophysics and Space Science, 1980
- The 10- and 20-?m interstellar absorption bands: Comparison with the infrared spectrum of the Nogoya meteoriteAstrophysics and Space Science, 1979
- Dust shell models for compact infrared sourcesThe Astrophysical Journal, 1977
- Radiative transfer in spherical circumstellar dust envelopes. V - Theoretical circumstellar graphite and silicate emission spectraThe Astrophysical Journal, 1976
- BRACKETT-alpha Emission in the Becklin-Neugebauer ObjefctThe Astrophysical Journal, 1976
- The 8-13 micron spectra of compact H II regionsThe Astrophysical Journal, 1975
- Circumstellar grains and the intrinsic polarization of starlightThe Astrophysical Journal, 1975
- Infrared spectra of silicate grainsAstronomische Nachrichten, 1971