Published June 1976
| Version v1
Journal article
The formation of interstellar molecules
Description
Cosmic rays may provide the energy flux necessary for the continual synthesis of molecules in dense H2 clouds, according to this detailed model of the carbon, oxygen, hydrogen and nitrogen chemistry of those regions
Additional details
Identifiers
- DOI
- 10.1063/1.3023517;
Publishing Information
- Journal Title
- Physics Today
- Journal Volume
- 29
- Journal Issue
- 6
- Series
- Phys. Today.
- Journal Page Range
- 32-39
- ISSN
- 0031-9228
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 7266911
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CARBON; COSMIC GASES; COSMIC RADIATION; COSMOCHEMISTRY; DEUTERIUM; HYDROGEN; H1 REGIONS; INTERSTELLAR SPACE; LIFETIME; MOLECULES; NITROGEN; OXYGEN; SPECTRA; SYNTHESIS
- Descriptors DEC
- CHEMISTRY; COSMIC RADIO SOURCES; ELEMENTS; FLUIDS; GASES; HYDROGEN ISOTOPES; IONIZING RADIATIONS; ISOTOPES; LIGHT NUCLEI; NONMETALS; NUCLEI; ODD-ODD NUCLEI; RADIATIONS; SPACE; STABLE ISOTOPES
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent