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相关论文: Binaries in the Hipparcos data: Keep digging

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Results of an archival survey are presented using B-band imaging of the eastern spiral arm of M31. Focusing on the eclipsing binary star population, a matched-filter technique has been used to identify 280 binary systems. Of these, 127…

天体物理学 · 物理学 2007-05-23 Ian Todd , Don Pollacco , Ian Skillen , D. M. Bramich , Steve Bell , Thomas Augusteijn

We present the first results of a comprehensive census of the stellar content of the nearby OB associations based on Hipparcos positions, proper motions and parallaxes for 12842 candidate member stars distributed over 21 fields on the sky.…

天体物理学 · 物理学 2007-05-23 P. T. de Zeeuw , A. G. A. Brown , J. H. J. de Bruijne , R. Hoogerwerf , J. Lub , R. S. Le Poole , A. Blaauw

We review the properties and applications of binary and millisecond pulsars. Our knowledge of these exciting objects has greatly increased in recent years, mainly due to successful surveys which have brought the known pulsar population to…

天体物理学 · 物理学 2016-11-23 D. R. Lorimer

It is difficult to discover pulsars via their gamma-ray emission because current instruments typically detect fewer than one photon per million rotations. This creates a significant computing challenge for isolated pulsars, where the…

高能天体物理现象 · 物理学 2020-10-23 L. Nieder , B. Allen , C. J. Clark , H. J. Pletsch

The Gliese 581 planetary system has received attention because it has been proposed to host a low-mass planet in its habitable zone. We re-analyse the radial velocity measurements reported to contain six planetary signals to see whether…

地球与行星天体物理 · 物理学 2015-05-27 Mikko Tuomi

We present a catalogue containing 839 candidate post common envelope systems. Common envelope evolution is very important in stellar astrophysics, particularly in the context of very compact and short-period binaries, including cataclysmic…

太阳与恒星天体物理 · 物理学 2021-10-27 Matthias U. Kruckow , Patrick G. Neunteufel , Rosanne Di Stefano , Yan Gao , Chiaki Kobayashi

The estimation of the binary fraction of hot subdwarfs is key to shed light on the different evolution scenarios proposed to explain the loss of the hydrogen envelope during the red giant branch phase. In this paper we analyse the spectral…

太阳与恒星天体物理 · 物理学 2022-06-22 E. Solano , A. Ulla , E. Pérez-Fernández , C. Rodrigo , R. Oreiro , A. Aller , M. Manteiga , R. Santoveña-Gómez , M. A. Álvarez , C. Dafonte

The results of an adaptive optics survey of exoplanet host stars for stellar companions is presented. We used the AEOS Telescope and its adaptive optics system to collect deep images of the stars in $I$-band. Sixty-two exoplanet host stars…

太阳与恒星天体物理 · 物理学 2015-05-30 Lewis C. Roberts , Nils H. Turner , Theo A. ten Brummelaar , Brian D. Mason , William I. Hartkopf

Finding pulsars in binaries are important for measurements of the masses of neutron stars, for tests of gravity theories, and for studies of star evolution. We are carrying out the Galactic Plane Pulsar Snapshot survey (GPPS) by using the…

高能天体物理现象 · 物理学 2025-02-07 P. F. Wang , J. L. Han , Z. L. Yang , T. Wang , C. Wang , W. Q. Su , J. Xu , D. J. Zhou , Yi Yan , W. C. Jing , N. N. Cai , J. P. Yuan , R. X. Xu , H. G. Wang , X. P. You

Virtually all binaries consisting of a white dwarf with a non-degenerate companion can be classified as either close post-interaction systems (with orbital periods of a few days or less), or wide systems (with periods longer than decades),…

We present orbital elements and mass sums for eighteen visual binary stars of spectral types B to K (five of which are new orbits) with periods ranging from 20 to more than 500 yr. For two double-line spectroscopic binaries with no previous…

太阳与恒星天体物理 · 物理学 2017-10-25 Rene A. Mendez , Ruben M. Claveria , Marcos E. Orchard , Jorge F. Silva

One notable example of exoplanet diversity is the population of circumbinary planets, which orbit around both stars of a binary star system. There are so far only 16 known circumbinary exoplanets, all of which lie in the same orbital plane…

地球与行星天体物理 · 物理学 2025-04-17 Thomas A. Baycroft , Lalitha Sairam , Amaury H. M. J Triaud , Alexandre C. M. Correia

We present relative positions of visual binaries observed during 2009 with the FastCam "lucky-imaging" camera at the 1.5-m Carlos Sanchez Telescope (TCS) at the Observatorio del Teide. We obtained 424 CCD observations (averaged in 198 mean…

太阳与恒星天体物理 · 物理学 2015-05-30 F. M. Rica , R. Barrena , G. Vazquez , J. A. Henriquez , F. Hernandez

We have measured the orbital parameters of seven close binaries, including six new objects, in a radial velocity survey of 38 objects comprising a hot subdwarf star with orbital periods ranging from ~0.17 to 3 d. One new system, GALEX…

太阳与恒星天体物理 · 物理学 2015-05-27 A. Kawka , S. Vennes , S. O'Toole , P. Nemeth , D. Burton , E. Kotze , D. A. H. Buckley

Using adaptive optics we study the binary population in the nearby OB association Scorpius OB2. We present the first results of our near-infrared adaptive optics survey among 199 (mainly) A- and B-type stars in Sco OB2. In total 151…

We report 370 measures of 170 components of binary and multiple star systems, obtained from speckle imaging observations made with the Differential Speckle Survey Instrument at Lowell Observatory's Discovery Channel Telescope in 2015…

Searches for planetary transits find many astrophysical false positives as a by-product. There are four main types analyzed in the literature: a grazing-incidence eclipsing binary star, an eclipsing binary star with a small radius companion…

太阳与恒星天体物理 · 物理学 2016-08-14 Radosław Poleski , Peter R. McCullough , Jeff A. Valenti , Christopher J. Burke , Pavel Machalek , Kenneth Janes

We have compiled a catalogue of eclipsing variable stars, the largest catalogue, containing classified eclipsing binaries. A procedure for the classification of eclipsing binaries, based on the catalogued data, is also developed. It was…

太阳与恒星天体物理 · 物理学 2013-06-20 Oleg Malkov , Ekaterina Avvakumova

Asteroids with companions constitute an excellent sample for studying the collisional and dynamical evolution of minor planets. The currently known binary population were discovered by different complementary techniques that produce, for…

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