Published August 1, 1976
| Version v1
Journal article
IRC+10 420: A hot supergiant maser
Creators
- 1. Theoretical Division, Los Alamos Scientific Laboratory
Description
IRC+10 420, of spectral type F8 Ia, is a maser in the OH molecule's ground-state lines at 1612, 1665, and 1667 MHz. Two 1612 MHz components are separated by 58 km s-1, with peak fluxes of 47 and 7 Jy. Upper limits are given for the 1720 MHz OH line and the 22,235 MHz H2O line. New infrared data are also presented
Additional details
Identifiers
- DOI
- 10.1086/182211;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 207
- Journal Issue
- 3
- Series
- Astrophys. J., Lett.
- Journal Page Range
- L195
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 8288428
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- GROUND STATES; HYDROXIDES; INFRARED SPECTRA; MASERS; RADIAL VELOCITY; SUPERGIANT STARS
- Descriptors DEC
- AMPLIFIERS; ELECTRONIC EQUIPMENT; ENERGY LEVELS; GIANT STARS; HYDROGEN COMPOUNDS; MICROWAVE AMPLIFIERS; MICROWAVE EQUIPMENT; OXYGEN COMPOUNDS; SPECTRA; STARS; VELOCITY
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent