Published November 1988
| Version v1
Journal article
Abundances of elements of the palladium group in the atmospheres of evolved stars. I. Molybdenum
Creators
Description
The abundance of molybdenum in the atmospheres of the K giants υ Ser, 9 Boo, and ρ Boo has been determined using spectra with reciprocal dispersion 6 angstrom/mm and the method of model atmospheres. Data on the abundance of this element in the atmospheres of other evolved stars are also given
Additional details
Publishing Information
- Journal Title
- Astrophysics (English Translation)
- Journal Volume
- 28
- Journal Issue
- 3
- Series
- Astrophysics (Engl. Transl.).
- Journal Page Range
- 354-356
- ISSN
- 0004-6396
- CODEN
- ATPYA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20082125
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Translation
- Descriptors DEI
- CHEMICAL COMPOSITION; EXCITATION; FLOW RATE; GIANT STARS; GRAVITATIONAL FIELDS; LINE WIDTHS; MOLYBDENUM; NUCLEOSYNTHESIS; SPECTRA; SPECTROSCOPIC CURVE OF GROWTH; STAR EVOLUTION; STAR MODELS; STELLAR ATMOSPHERES; TEMPERATURE DISTRIBUTION; TURBULENCE
- Descriptors DEC
- ATMOSPHERES; DIAGRAMS; ELEMENTS; ENERGY-LEVEL TRANSITIONS; INFORMATION; MATHEMATICAL MODELS; METALS; OPTICAL DEPTH CURVE; STARS; SYNTHESIS; TRANSITION ELEMENTS
Optional Information
- Notes
- Translated from Astrofizika; 28: No. 3, 595-598(May-Jun 1988). Cover-to-cover translation of Astrofizika (USSR).