Published February 1977
| Version v1
Journal article
The central star of NGC 1360: a spectroscopic binary within a planetary nebula
Creators
- 1. Instituto de Astronomia y Fisica del Espacio, Buenos Aires (Argentina)
Description
CPD - 260389, a hot subdwarf at the centre of the planetary nebula NGC 1360, is shown to be a single-lined spectroscopic binary with a period of about 8 day. The primary (visible) component appears to be less massive than its companion, and the total stellar mass of the system is presumably below one solar mass. (author)
Additional details
Identifiers
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 178
- Journal Issue
- 3
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 409-414
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 8308641
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BINARY STARS; DWARF STARS; PLANETARY NEBULAE; SPECTRA; VARIABLE STARS
- Descriptors DEC
- NEBULAE; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent