Published October 15, 1973
| Version v1
Journal article
Anomalous 1720-MHz OH emission from V1057 Cygni
Creators
- 1. Department of Physics and Research Laboratory of Electronics, Massachusetts Institute of Technology
Description
We detected a new type of OH ermssion source from the V1057 Cyg star position. Only the 1 720-MHz line is observable in emission. The line can be decomposed into two Gaussian cornponents, each with a line width at half-power of about 0.3 km s-i, separated by about 0.3 km -i Both components are elliptically polarized. Subject headings:spectra, radio - star formation - stars, individual
Additional details
Additional titles
- Augmented title (English)
- Elliptically polarized, line width at half-power
Identifiers
- DOI
- 10.1086/181323;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 185
- Journal Issue
- 2
- Series
- Astrophys. J., Lett.
- Journal Page Range
- L71
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 5142569
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ENERGY SPECTRA; HYDROXYL RADICALS; LINE WIDTHS; RADIOWAVE RADIATION; STAR EVOLUTION; STARS; STOKES PARAMETERS
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; RADIATIONS; RADICALS; SPECTRA
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent