Published January 15, 1977
| Version v1
Journal article
On the relationship between the infrared source CRL 2591 (UOA-27) and its radio and H2O counterparts
Creators
- 1. California Institute of Technology
Description
New radio, infrared, and H2O maser observations show that there is a 7'' angular separation between the protostar-like infrared source CRL 2591 and the compact H II region which has until now been identified with it, while the H2O maser coincides with the infrared source. This result, together with an extension of photometric measurements to 20 μm and a much improved upper limit to its angular size, reinforces the apparent similarity of CRL 2591 to the BN object in Orion and to W3/IRS 5
Additional details
Identifiers
- DOI
- 10.1086/182347;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 211
- Journal Issue
- 2
- Series
- Astrophys. J., Lett.
- Journal Page Range
- L89
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 8320011
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- H2 REGIONS; INFRARED RADIATION; INFRARED SPECTRA; MASERS; NEBULAE; PROTOSTARS; RADIOWAVE RADIATION
- Descriptors DEC
- AMPLIFIERS; COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; ELECTRONIC EQUIPMENT; MICROWAVE AMPLIFIERS; MICROWAVE EQUIPMENT; RADIATIONS; SPECTRA
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent