Royal Astronomical Society | 2015 Apr 01
Many, perhaps most, stars in the Universe live their lives with companions by their sides – in so-called binary systems. Until recently, however, the ancient RR Lyrae stars appeared, for mysterious reasons, to live their lives all alone. A recent study led by Chilean astronomers shows that RR Lyrae stars may not be as lonely as previously thought. The new research is published in Monthly Notices of the Royal Astronomical Society Letters.
- [i]Map of the sky towards the central bulge of the Milky Way, with the positions of the binary candidates indicated as red circles. The background image is based on near-infrared observations obtained in the course of the[/i] [url=http://www.eso.org/public/news/eso1242/][i]Vista Variables in the Vía Láctea (VVV) ESO Public Survey[/i][/url]. [i]The scale is approximately 20 by 15 degrees. [b](Credit: D. Minniti)[/b][/i]
Stars are very often found not in isolation, but rather in pairs. In these so-called binary systems, two stars orbit around their common centre of gravity. Suitable binary systems are of extreme importance in astrophysics, as their properties can be inferred with unparalleled accuracy from detailed analysis of their orbital properties.
Puzzlingly, however, an overwhelming majority of the known members of a very important family of stars, known to astronomers as RR Lyrae variables, have for long appeared to live their lives all alone. These stars, being among the oldest known in the cosmos, contain precious information about the origin and evolution of the stellar systems that harbour them, such as the Milky Way itself. However, the lack of RR Lyrae stars in binary systems has made a direct assessment of some of their key properties difficult. Most often, theory had to be invoked to fill the gap. ...
New RR Lyrae variables in binary systems - G. Hajdu et al
- Monthly Notices of the RAS Letters 449(1) L113 (2015 May 01) DOI: 10.1093/mnrasl/slv024
arXiv.org > astro-ph > arXiv:1502.01318 > 04 Feb 2015