On statistical distributions of wide binary stars

dc.contributor.author	Chulkov, D.A.
dc.contributor.author	Trushin, D.I.
dc.date.accessioned	2017-06-04T18:30:12Z
dc.date.available	2017-06-04T18:30:12Z
dc.date.issued	2012
dc.identifier.citation	On statistical distributions of wide binary stars / D.A. Chulkov, D.I. Trushin // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 23-24. — Бібліогр.: 6 назв. — англ.	uk_UA
dc.identifier.issn	2227-1481
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/119164
dc.description.abstract	The semi-major axis is a key parameter of binary stellar systems. In order to obtain current semi-major axis distribution we investigated a volume-limited sample of the binaries in solar neighbourhood. Obtained distribution shows unsatisfactory agreement with the canonical Opik's law.	uk_UA
dc.description.sponsorship	Authors thank Oleg Yu. Malkov, Anastasia Isaeva, Alexey S. Rastorguev and Leonid Zotov for their indispensable contribution in this research.	uk_UA
dc.language.iso	en	uk_UA
dc.publisher	Головна астрономічна обсерваторія НАН України	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.title	On statistical distributions of wide binary stars	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA