Published June 1, 1974 | Version v1
Journal article Metadata-only

34-micron observations of eta Carinae, G333.6 to 0.2, and the galactic center

Creators

  • 1. California Inst. of Tech., Pasadena

Description

Preliminary 3 observations show that (a) the majority of the infrared flux from Carinae can be attributed to a 250 K circumstellar dust shell, (b) the infrared energy distribution of G333.6-0.2 exhibits a smooth continuum rising to 34,o, and (c) the central 30" area of the galactic center is a strong 34i emitter with an energy distribution similar to that of G333.6-0.2. Subject headings: circumstellar shells - Galaxy, The - infrared sources - nebulae

Additional details

Identifiers

DOI
10.1086/181507;

Publishing Information

Journal Title
The Astrophysical Journal
Journal Volume
190
Journal Issue
2
Series
Astrophys. J., Lett.
Journal Page Range
L69
ISSN
0004-637X

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
6164175
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
No Abstract
Descriptors DEI
COSMIC DUST; DISTRIBUTION; EMISSION SPECTRA; ENERGY SPECTRA; FLUX DENSITY; INFRARED RADIATION; MILKY WAY; SHELLS; STARS
Descriptors DEC
DUSTS; ELECTROMAGNETIC RADIATION; GALAXIES; RADIATIONS; SPECTRA

Optional Information

Notes
Published in summary form only.; Updated automatically by Metadata and Full-Text Enrichment Agent