Published February 15, 1975
| Version v1
Journal article
Very long baseline interferometric observations of OH/IR stars
Creators
- 1. Owens Valley Radio Observatory and Division of Geological and Planetary Sciences, California Institute of Technology
Description
Very long baseline interferometric observations of five type II OH/IR objects indicate that the apparent size of the masing components is greater than approx.0''.1. The present observations, combined with current theories, indicate that the 1612-MHz OH maser associated with Mira variables originates in the outer regions of the circumstellar dust
Additional details
Identifiers
- DOI
- 10.1086/181738;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 196
- Journal Issue
- 1
- Series
- Astrophys. J., Lett.
- Journal Page Range
- L35
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 6203062
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC DUST; COSMIC RADIO SOURCES; INFRARED RADIATION; LUMINOSITY; SPECTRA; VARIABLE STARS
- Descriptors DEC
- DUSTS; ELECTROMAGNETIC RADIATION; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent