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Binary systems have long been recognized as the source of powerful astrophysical diagnostics. Among the many applications of binary stars, they have been used as probes of stellar structure and evolution (both of single and binary stars) in…

天体物理学 · 物理学 2007-05-23 Ignasi Ribas

Context. Binary asteroids are present in all populations of the Solar System, from near-Earth to trans-Neptunian regions. As is true for the small Solar System bodies (SSSBs), binary asteroids generally offer valuable insights into the…

地球与行星天体物理 · 物理学 2025-03-18 Ziyu Liu , Daniel Hestroffer , Josselin Desmars , Pedro David

I list the 16 planetary nebulae (PNe) known to contain close-binary nuclei, and show that the nebulae generally have axisymmetric structures, including elliptical, bipolar, or ring morphologies. The orbital periods range from 2.7 hr to 16…

天体物理学 · 物理学 2007-05-23 Howard E. Bond

We report on a high-spatial-resolution survey for binary stars in the periphery of the Orion Nebula Cluster, at 5 - 15 arcmin (0.65 - 2 pc) from the cluster center. We observed 228 stars with adaptive optics systems, in order to find…

For three decades, adaptive optic surveys have revealed an excess of T Tauri binaries across a = 10-100 au in nearby star-forming regions compared to the field population of main-sequence (MS) stars. Such an excess requires that most stars…

太阳与恒星天体物理 · 物理学 2025-08-04 Caleb Eastlund , Maxwell Moe , Kaitlin M. Kratter , Marina Kounkel

In this review paper, we summarise the goals of asteroseismic studies of close binary stars. We first briefly recall the basic principles of asteroseismology, and highlight how the binarity of a star can be an asset, but also a…

天体物理学 · 物理学 2009-11-13 Conny Aerts

We report the discovery of a planetary nebula centered on the poorly studied symbiotic binary star DT Ser. In a few other symbiotic stars spatially resolved nebulae have been discovered: however, only one of them might be a genuine…

太阳与恒星天体物理 · 物理学 2015-06-16 U. Munari , R. L. M. Corradi , A. Siviero , L. Baldinelli , A. Maitan

We present a list of delta Scuti stars in double and multiple systems, ranging from the very wide binaries to the very close ones such as spectroscopic and eclipsing systems including the optical visual pairs which are of no further use…

天体物理学 · 物理学 2007-05-23 P. Lampens , H. M. J. Boffin

The discovery of binaries in each of the major populations of minor bodies in the solar system is propelling a rapid growth of heretofore unattainable physical information. The availability of mass and density constraints for minor bodies…

天体物理学 · 物理学 2009-11-11 Keith S. Noll

A number of efforts are underway to detect close binary stars in planetary nebulae. The primary goal of these studies is to determine the binary fraction of central stars. The next stage is a detailed analysis of the binaries to determine…

太阳与恒星天体物理 · 物理学 2010-10-08 Todd C. Hillwig

This paper reviews current knowledge of symbiotic binaries, with special emphasis on their multifrequency observational characteristics, and basic parameters of the symbiotic system components. We start with a brief presentation of variable…

天体物理学 · 物理学 2007-05-23 Joanna Mikolajewska

Symbiotic stars are long-period interacting binary systems in which an evolved red giant star transfers material to its much hotter compact companion. Such a composition places them among the most variable stars. In addition to periodic…

天体物理学 · 物理学 2007-05-23 Joanna Mikolajewska

Close, compact, hierarchical, multiple stellar systems, i.e., multiples having an outer orbital period from months to a few years, comprise a small, but continuously growing group of the triple and multiple star zoo. Many of them consist of…

太阳与恒星天体物理 · 物理学 2022-01-05 Tamás Borkovits

We present the results of an expanded, long-term radial velocity search (25 yrs) for evidence of binarity in a sample of seven bright proto-planetary nebulae (PPNe). The goal is to investigate the widely-held view that the bipolar or…

太阳与恒星天体物理 · 物理学 2017-09-12 Bruce J. Hrivnak , Griet Van de Steene , Hans Van Winckel , Julius Sperauskas , David Bohlender , Wenxian Lu

We have carried out a major survey for visual binaries towards the Orion Nebula Cluster using HST images obtained with an H-alpha filter. Among 781 likely ONC members more than 60" from theta-1 Ori C, we find 78 multiple systems (75…

天体物理学 · 物理学 2009-06-23 Bo Reipurth , Marcelo M. Guimarães , Michael S. Connelley , John Bally

During the last years, many observational studies have revealed that binaries play an active role in the shaping of non spherical planetary nebulae. We review the different works that lead to the direct or indirect evidence for the presence…

太阳与恒星天体物理 · 物理学 2014-10-15 Eric Lagadec , Olivier Chesneau

Close-binary central stars of planetary nebulae offer a unique tool with which to study the critical and yet poorly understood common-envelope phase of binary stellar evolution. Furthermore, as the nebula itself is thought to comprise the…

太阳与恒星天体物理 · 物理学 2024-12-13 David Jones

We have used the NICMOS NIC1 camera on the Hubble Space Telescope to obtain high angular resolution images of 51 ultracool dwarfs in the immediate Solar Neighbourhood. Nine systems are resolved as binary, with component separations from 1.5…

天体物理学 · 物理学 2008-11-26 I. N. Reid , E. Lewitus , P. R. Allen , Kelle L. Cruz , Adam J. Burgasser

Be/X-ray binary systems provide an excellent opportunity to study the physics around neutron stars through the study of the behaviour of matter around them. Intermediate and low-luminosity type outbursts are interesting because they provide…

高能天体物理现象 · 物理学 2019-08-15 M. D. Caballero-Garcia , A. Camero-Arranz , M. Ozbey Arabaci , R. Hudec

We describe some recent nonlinear three dimensional hydrodynamic simulations of accretion discs in binary systems where the orbit is circular and not necessarily coplanar with the disc midplane. The calculations are relevant to a number of…

天体物理学 · 物理学 2009-10-30 J. C. B. Papaloizou , J. D. Larwood , R. P. Nelson , C. Terquem