Hostname: page-component-745bb68f8f-mzp66 Total loading time: 0 Render date: 2025-02-03T08:53:43.741Z Has data issue: false hasContentIssue false
  • English
  • Français

The Magnetic Field of the Galaxy in the Solar Vicinity and the Polarization of Stars

Published online by Cambridge University Press:  19 July 2016

A.N. Makarov  and
R.R. Andreassian
A.N. Makarov
Affiliation:
1. Byurakan Astrophysical Observatory, 378433 Armenia, USSR 2. Buryat Pedagogical Institute, 670000 Ulan-Ude, Buryatia, USSR
R.R. Andreassian
Affiliation:
1. Byurakan Astrophysical Observatory, 378433 Armenia, USSR

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The results of a study of the magnetic field of the Galaxy up to ~3.5 kpc from the Sun by the analysis of interstellar polarization of optical radiation of catalogue stars (Mathewson et al., 1978) are presented. For the regions 90° < l <180° and 300° < l < 360°, where the polarization degree P is maximum, the empirical form is found.

Type
2. The Magnetic Field Structure of the Milky Way: The Meeting of Observation and Theory
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 65 - 66
Copyright
Copyright © Kluwer 1990 

References

Andreassian, R.R. and Makarov, A.N. (1989) Astrofizika (in press).Google Scholar
Mathewson, D.S., Ford, V.L. and Krautter, Y. (1978) Bulletin CDS 14, 115.Google Scholar
Sofue, Y. and Fujimoto, M. (1983) Astrophys. J. 265, 722.Google Scholar