Published 1972
| Version v1
Journal article
Recent work on interstellar grains
Description
Observational data accumulated over the past decade have considerably narrowed down the choice of proposals for grain models. Mixtures of particles composed of refractory species such as graphite, silicates, quartz and iron appear likely. Such particles may form in a wide range of astronomical situations, for example, cool stars, protostars and supernovae explosions. Dust grains are responsible for infrared radiation in galactic sources, and also play an important role in the synthesis of interstellar molecules.
Additional details
Identifiers
Publishing Information
- Journal Title
- Reports on Progress in Physics
- Journal Volume
- 35
- Journal Issue
- 1
- Series
- Rep. Progr. Phys.
- Journal Page Range
- 157-234
- ISSN
- 0034-4885
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 4035767
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTRONOMY; COSMIC DUST; DATA ACQUISITION; FUNCTIONAL MODELS; GALAXIES; GRAPHITE; INFRARED RADIATION; INTERSTELLAR SPACE; IRON; MIXTURES; PARTICLES; QUARTZ; REFRACTORIES; SILICATES; SUPERNOVAE
- Descriptors DEC
- CARBON; DISPERSIONS; DUSTS; ELECTROMAGNETIC RADIATION; ELEMENTS; METALS; NONMETALS; OXIDES; RADIATIONS; SILICON COMPOUNDS; SILICON OXIDES; SPACE; STARS; TRANSITION ELEMENTS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent