arXiv Open Access 2017

Open star clusters and Galactic structure

Y. C. Joshi
Lihat Sumber

Abstrak

In order to understand the Galactic structure, we perform a statistical analysis of the distribution of various cluster parameters based on an almost complete sample of Galactic open clusters yet available. The geometrical and physical characteristics of a large number of open clusters given in the MWSC catalogue are used to study the spatial distribution of clusters in the Galaxy and determine the scale height, solar offset, local mass density and distribution of reddening material in the solar neighbourhood. We also explored the mass-radius and mass-age relations in the Galactic open star clusters. We find that the estimated parameters of the Galactic disk are largely influenced by the choice of cluster sample.

Topik & Kata Kunci

Penulis (1)

Y

Y. C. Joshi

Format Sitasi

Joshi, Y.C. (2017). Open star clusters and Galactic structure. https://arxiv.org/abs/1707.09126

Akses Cepat

Lihat di Sumber
Informasi Jurnal
Tahun Terbit
2017
Bahasa
en
Sumber Database
arXiv
Akses
Open Access ✓