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Infrared studies of dust grains in infrared reflection nebulae
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Werner, Michael W. Pendleton, Yvonne J. Tielens, Alexander G. G. M. |
| Copyright Year | 1989 |
| Description | IR reflection nebulae, regions of dust which are illuminated by nearby embedded sources, were observed in several regions of ongoing star formation. Near IR observation and theoretical modelling of the scattered light form IR reflection nebulae can provide information about the dust grain properties in star forming regions. IR reflection nebulae were modelled as plane parallel slabs assuming isotropically scattering grains. For the grain scattering properties, graphite and silicate grains were used with a power law grain size distribution. Among the free parameters of the model are the stellar luminosity and effective temperature, the optical depth of the nebula, and the extinction by foreground material. The typical results from this model are presented and discussed. |
| File Size | 101936 |
| Page Count | 2 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19910005657 |
| Archival Resource Key | ark:/13960/t5q866v4b |
| Language | English |
| Publisher Date | 1989-12-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Grain Size Size Distribution Scattering Ice Silicates Stellar Luminosity Near Infrared Radiation Cosmic Dust Star Formation Interstellar Extinction Graphite Mathematical Models Optical Thickness Interstellar Matter Reflection Nebulae Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |