Article contents
Dynamic study of possible host stars for extrasolar planetary systems
Published online by Cambridge University Press: 05 January 2015
Abstract
We present the stellar systems which consist of double and multiple stars with distances 3.5 ÷ 25 pc from the Sun, belonging to spectral classes F, G, K, M, having masses from 0.3 to 1.5 solar mass and can, in principle, possess planetary systems. On the basis of observations with Pulkovo 65 cm refractor the relative positions of double stars, the parameters of motion, the orbits and also the ephemeris for the nearest epochs have been computed.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 9 , Issue S310: Complex Planetary Systems , July 2014 , pp. 104 - 105
- Copyright
- Copyright © International Astronomical Union 2014
References
- 2
- Cited by