Published July 1, 1977
| Version v1
Journal article
Far-infrared emission from compact sources in NGC 2264 and the rosette nebula
Creators
- 1. Steward Observatory, University of Arizona
Description
Far-infrared observations are reported of known2--20 μm sources in NGC 2264 and the Rosette Nebula. Both sources are unresolved in the far-infrared with sizes 9 or approx. =20''. Both have relatively cool 53--175μm colors. The observed infrared luminosities of a few times 103L/sub sun/and the lack of radio continuum emission suggest that both sources may be stellar or protostellar objects of a moderate mass, approx.5--10M/sub sun/of the carbon is found in CO molecules
Additional details
Identifiers
- DOI
- 10.1086/155341;
Publishing Information
- Journal Title
- The Astrophysical Journal
- Journal Volume
- 215
- Journal Issue
- 1
- Series
- Astrophys. J.
- Journal Page Range
- 151
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 9351020
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BLACK HOLES; GALACTIC EVOLUTION; GALAXIES; GALAXY CLUSTERS; INFRARED RADIATION; ROTATION; SPHERICAL MODEL; STAR ACCRETION; STAR CLUSTERS
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; MATHEMATICAL MODELS; NUCLEAR MODELS; RADIATIONS; STAR EVOLUTION
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent