CrossRef
Open Access
2016
Orbits of Wide Binaries – New Possibilities
Olga V. Kiyaeva
Abstrak
Abstract We use the Apparent Motion Parameters (AMP) method for the determination of orbits of visual double stars (Kiselev & Kiyaeva 1980). The quality of AMP orbits is completely dependent on the precision of parameters of relative positions and motions at the same instant. They are calculated on the basis of a short arc of observations. To determine these parameters, we use recent high precision observations obtained with the best modern techniques. New orbits of three stars are presented.
Penulis (1)
O
Olga V. Kiyaeva
Akses Cepat
Informasi Jurnal
- Tahun Terbit
- 2016
- Bahasa
- en
- Sumber Database
- CrossRef
- DOI
- 10.1515/astro-2017-0136
- Akses
- Open Access ✓