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相关论文: Does ADS 9346 have a low-mass companion?

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Star ADS 9173=WDS 14135+5147=Hip 69483 is a complex system. The B component has a spectroscopic companion, whose orbit with a period of 4.9 years has been known since 1986. The Gaia telescope has detected a distant faint pair over 100…

太阳与恒星天体物理 · 物理学 2023-08-01 O. V. Kiyaeva , I. S. Izmailov , N. V. Narizhnaya , L. G. Romanenko

We report the discovery of a low-mass companion to HR3549, an A0V star surrounded by a debris disk with a warm excess detected by WISE at 22 $\mu$m ($10\sigma$ significance). We imaged HR3549 B in the L-band with NAOS-CONICA, the adaptive…

Eps Ind A is one of the nearest sun-like stars, located only 3.6 pc away. It is known to host a binary brown dwarf companion, Eps Ind Ba/Bb, at a large projected separation of 6.7", but radial velocity measurements imply that an additional,…

地球与行星天体物理 · 物理学 2015-05-13 M. Janson , D. Apai , M. Zechmeister , W. Brandner , M. Kuerster , M. Kasper , S. Reffert , M. Endl , D. Lafreniere , K. Geissler , S. Hippler , Th. Henning

In our ongoing deep infrared imaging search for faint wide secondaries of planet-candidate host stars we have confirmed astrometrically the companionship of a low-mass object to be co-moving with HD89744, a companion-candidate suggested…

天体物理学 · 物理学 2015-06-24 M. Mugrauer , R. Neuhäuser , T. Mazeh , E. Guenther , M. Fernández

We have observed 49 X-ray detected bright late B-type dwarfs to search for close low-mass pre-main sequence (PMS) companions using the European Southern Observatory's ADONIS (Adaptive Optics Near Infrared System) instrument. We announce the…

天体物理学 · 物理学 2009-11-06 S. Hubrig , D. Le Mignant , P. North , J. Krautter

PSR J1906+0746 is a young pulsar in the relativistic binary with the second-shortest known orbital period, of 3.98 hours. We here present a timing study based on five years of observations, conducted with the 5 largest radio telescopes in…

We report the discovery of one possible neutron star binary ($P_{\rm orb} =$ 0.8666 day) by using the LAMOST low-resolution spectroscopic data. The visible companion is a late A-type dwarf ($T_{\rm eff} = 7900 \pm 200$ K; log$g$ $=$…

高能天体物理现象 · 物理学 2022-12-06 Hailong Yuan , Song Wang , Zhongrui Bai , Yue Wang , Yiqiao Dong , Mengxin Wang , Sicheng Yu , Yongheng Zhao , Yaoquan Chu , Jifeng Liu , Haotong Zhang

We report the discovery of a companion to the high proper motion star LHS 1589, a nearby high-velocity, low-mass subdwarf. The companion (LHS 1589B) is located 0.224+/-0.004" to the southwest of the primary (LHS 1589A), and is 0.5 magnitude…

天体物理学 · 物理学 2009-11-13 Sebastien Lepine , R. Michael Rich , Michael M. Shara , Kelle L. Cruz , Andrew Skemer

Most millisecond pulsars with low-mass companions are in systems with either helium-core white dwarfs or non-degenerate ("black widow" or "redback") stars. A candidate counterpart to PSR J1816+4510 was identified by Kaplan et al. (2012)…

太阳与恒星天体物理 · 物理学 2015-06-15 David L. Kaplan , Varun B. Bhalerao , Marten H. van Kerkwijk , Detlev Koester , Shri R. Kulkarni , Kevin Stovall

We present the results of an aperture masking interferometry survey for substellar companions around 67 members of the young (~8-200Myr) nearby (~5-86pc) AB Doradus, Beta Pictoris, Hercules-Lyra, TW Hya, and Tucana-Horologium stellar…

PSR J0636+5128 is a millisecond pulsar in one of the most compact pulsar binaries known, with a 96\,min orbital period. The pulsar mass function suggests a very low-mass companion, similar to that seen in so-called "black widow" binaries.…

高能天体物理现象 · 物理学 2018-09-05 D. L. Kaplan , K. Stovall , M. H. van Kerkwijk , C. Fremling , A. G. Istrate

Context. Brown dwarf companions to stars at separations of a few AU or less are rare objects, and none have been found so far around early-type M dwarfs M0V-M5V). With GJ 1046 (M2.5V), a strong candidate for such a system with a separation…

天体物理学 · 物理学 2009-11-13 M. Kürster , M. Endl , S. Reffert

We report spectroscopic observations of the star HIP 50796, previously considered (but later rejected) as a candidate member of the TW Hya association. Our measurements reveal it to be a single-lined binary with an orbital period of 570…

天体物理学 · 物理学 2008-11-26 Guillermo Torres

Stars of Pulkovo observatory program are observed on 65-cm refractor during many years for study their positions and movement. We represent example of two visual binary stars, for which orbits and masses of components were determined, and…

太阳与恒星天体物理 · 物理学 2018-08-15 N. A. Shakht , D. L. Gorshanov , O. O. Vasilkova

Recently, Gauza et al. (2015) reported the discovery of a companion to the late M-dwarf, VHS J125601.92-125723.9 (VHS 1256-1257). The companion's absolute photometry suggests its mass and atmosphere are similar to the HR 8799 planets.…

We present optical and near-infrared adaptive optics (AO) imaging and spectroscopy of 13 ultracool (>M6) companions to late-type stars (K7-M4.5), most of which have recently been identified as candidate members of nearby young moving groups…

We report the discovery of a dark companion to 2MASS J15274848+3536572 with an orbital period of 6.14 hr. Combining the radial velocity from LAMOST observations and modelling of the multiband light curve, one obtains a mass function of…

We report the detection of a substellar companion orbiting the G5 dwarf HD 16760 from the N2K sample. Precise Doppler measurements of the star from Subaru and Keck revealed a Keplerian velocity variation with a period of 466.47+-0.35 d, a…

We report the discovery of SDSS~J022932.28+713002.7, a nascent extremely low-mass (ELM) white dwarf (WD) orbiting a massive ($> 1\,M_\odot$ at 2$\sigma$ confidence) companion with a period of 36 hours. We use a combination of spectroscopy,…

We report the detection of a radial velocity companion to SDSS J091709.55+463821.8, the lowest mass white dwarf currently known with M~0.17Msun. The radial velocity of the white dwarf shows variations with a semi-amplitude of 148.8 km/s and…

天体物理学 · 物理学 2009-06-23 Mukremin Kilic , Warren R. Brown , Carlos Allende Prieto , M. H. Pinsonneault , S. J. Kenyon
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