Published 1973
| Version v1
Journal article
Dust in the core of the Small Magellanic Cloud
Creators
Description
Of 11 stars in the SMC core selected from UBV photometry as possibly reddened early-type stars, four appear to be members, one a Be star. The result is consistent with a normal dust content of the Cloud, but further photometry is desirable.
Additional details
Identifiers
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 161
- Journal Issue
- 1
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 5P-8P
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 4066205
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- No Abstract
- Descriptors DEI
- ABSORPTION; BRIGHTNESS; COLOR; COSMIC DUST; COSMIC GASES; HERTZSPRUNG-RUSSELL DIAGRAM; LUMINOSITY; MAGELLANIC CLOUDS; PHOTOMETRY; STARS; ULTRAVIOLET RADIATION; VISIBLE RADIATION
- Descriptors DEC
- DIAGRAMS; DUSTS; ELECTROMAGNETIC RADIATION; FLUIDS; GALAXIES; GASES; OPTICAL PROPERTIES; ORGANOLEPTIC PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS
Optional Information
- Notes
- Short communication.; Updated automatically by Metadata and Full-Text Enrichment Agent