Published February 1, 1973
| Version v1
Journal article
Stellar and interstellar K lines: gamma Pegasi and iota Herculis
Creators
Description
High-resolution scans show that the relatively strong ( 90 mA) K lines of Ca ii in the early B stars y Peg and L Her are almost entirely stellar in origin, although the latter case includes a small interstellar contribution. Such stellar lines can be of great importance in augmenting the interstellar absorption, up through the earliest of the B stars. Subject headings: early-type stars - interstellar matter line profiles stars, individual
Additional details
Identifiers
- DOI
- 10.1086/151918;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 179
- Journal Issue
- 3
- Series
- Astrophys. J.
- Journal Page Range
- 823
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 5092539
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CALCIUM IONS; INTERSTELLAR SPACE; PHOTOMETRY; STARS; X-RAY SPECTRA; X-RAY SPECTROMETERS
- Descriptors DEC
- CHARGED PARTICLES; IONS; MEASURING INSTRUMENTS; SPACE; SPECTRA; SPECTROMETERS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent