Published September 1980
| Version v1
Journal article
The distribution of main-sequence stars in the open cluster NGC 7789
Description
By star counts on four plates with different limiting magnitudes, it was found that the relative frequency of Main-Sequence stars increases from the centre of the cluster to the boundary. It is shown that the stars of NGC 7789 are separated according to their masses. (orig.)
Additional details
Publishing Information
- Journal Title
- Astrophys. Space Sci.
- Journal Volume
- 72
- Journal Issue
- 1
- Series
- Astrophys. Space Sci.
- Journal Page Range
- 233-236
- ISSN
- 0004-640X
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 12586920
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- DENSITY; MAIN SEQUENCE STARS; MASS; SPATIAL DISTRIBUTION; STAR CLUSTERS
- Descriptors DEC
- DISTRIBUTION; PHYSICAL PROPERTIES; STARS