Published 1976
| Version v1
Journal article
Planetary nebula in a red globular cluster in the Large Magellanic Cloud
Description
An object close to the center of the red LMC globular cluster NGC 1852 is shown to be a low-excitation planetary nebula and may be a cluster member. The nitrogen abundance of the shell is between 10 and 20 times less than the solar value. The similarity in the central star temperature of this planetary to that in M 15 is mentioned
Additional details
Identifiers
- DOI
- 10.1086/130007;
Publishing Information
- Journal Title
- Publications of the Astronomical Society of the Pacific
- Journal Volume
- 88
- Journal Issue
- 525
- Series
- Publ. Astron. Soc. Pac.
- Journal Page Range
- 669
- ISSN
- 0004-6280
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 8316989
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BALMER LINES; CHEMICAL COMPOSITION; MAGELLANIC CLOUDS; NITROGEN; PLANETARY NEBULAE; STAR CLUSTERS
- Descriptors DEC
- ELEMENTS; GALAXIES; NEBULAE; NONMETALS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent