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Related papers: Orbits of Six Late-type Active-Chromosphere Binari…

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We report on two RossiXTE observations of the anomalous X-ray pulsars 1E 1048.1-5937 and 1E 2259+586. Both sources have continued their almost constant spin-down during 1995/96. We carried out a search for orbital Doppler shifts, in their…

Astrophysics · Physics 2009-10-30 S. Mereghetti , G. L. Israel , L. Stella

Differential astrometry measurements from the Palomar High-precision Astrometric Search for Exoplanet Systems have been combined with lower precision single-aperture measurements covering a much longer timespan (from eyepiece measurements,…

Close binary interactions may play a critical role in the formation of the rapidly rotating Be stars. Mass transfer can result in a mass gainer star spun up by the accretion of mass and angular momentum, while the mass donor is stripped of…

Solar and Stellar Astrophysics · Physics 2023-04-26 Luqian Wang , Douglas R. Gies , Geraldine J. Peters , Zhanwen Han

Orbital elements are presented for the Tc-poor S stars HR 363 (= HD 7351) and HD 191226. With an orbital period of 4592 d (=12.6 y), HR 363 has the longest period known among S stars, and yet it is a strong X-ray source. Its X-ray flux is…

Astrophysics · Physics 2009-10-30 J. M. Carquillat , A. Jorissen , S. Udry , N. Ginestet

Long-term precise Doppler measurements with the CORALIE spectrograph reveal the presence of a second planet orbiting the solar-type star HD202206. The radial-velocity combined fit yields companion masses of m_2\sini = 17.4 M_Jup and 2.44…

Astrophysics · Physics 2015-06-24 A. C. M. Correia , S. Udry , M. Mayor , J. Laskar , D. Naef , F. Pepe , D. Queloz , N. C. Santos

With Hubble Space Telescope Fine Guidance Sensor astrometry and previously published radial velocity measures we explore the exoplanetary system HD 202206. Our modeling results in a parallax, $\pi_{abs} = 21.96\pm0.12$ milliseconds of arc,…

Solar and Stellar Astrophysics · Physics 2017-05-31 G. Fritz Benedict , Thomas E. Harrison

While monitoring a sample of apparently slowly rotating superficially normal bright late B and early A stars in the northern hemisphere, we have discovered that HD 67044 and HD 42035, hitherto classified as normal late B-type stars, are…

Solar and Stellar Astrophysics · Physics 2016-04-13 R. Monier , M. Gebran , F. Royer

We report the discovery of faint common-proper-motion companions to the nearby southern solar-type stars HD43162, HD67199, HD114837, HD114853, HD129502, HD165185, HD197214, and HD212330 from near-infrared imaging and astrometry. We also…

Solar and Stellar Astrophysics · Physics 2015-06-17 R. Chini , K. Fuhrmann , A. Barr Domínguez , F. Pozo Nuñez , C. Westhues , K. Hodapp

We present new, high-precision Doppler radial velocity (RV) data sets for the nearby K3V star HD 219134. The data include 175 velocities obtained with the HIRES Spectrograph at the Keck I Telescope, and 101 velocities obtained with the Levy…

Aims. We present the results obtained from a long-term spectroscopic campaign devoted to the multiplicity of O-type stars in the young open cluster NGC2244 and in the Mon OB2 association. Methods. Our spectroscopic monitoring was performed…

Solar and Stellar Astrophysics · Physics 2020-12-09 L. Mahy , Y. Naze , G. Rauw , E. Gosset , M. De Becker , H. Sana , P. Eenens

We have used the radial velocity variations of two sdB stars previously reported to be binaries to establish their orbital periods. They are PG0940+068, (P=8.33d) and PG1247+554 (P=0.599d). The minimum masses of the unseen companions,…

Astrophysics · Physics 2009-10-31 P. F. L. Maxted , C. K. J. Moran , T. R. Marsh , A. A. Gatti

Radial-velocity measurements and sine-curve fits to the orbital velocity variations are presented for the seventh set of ten close binary systems: V410 Aur, V523 Cas, QW Gem, V921 Her, V2357 Oph, V1130 Tau, HN UMa, HX UMa, HD 93917, NSV…

Periods, eccentricities, and masses in hierarchical stellar systems inform us on the formation and early evolution of these fascinating objects. To complement the multiplicity statistics of nearby solar-type stars, 19 new spectroscopic…

Solar and Stellar Astrophysics · Physics 2022-03-30 Andrei Tokovinin

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…

Solar and Stellar Astrophysics · Physics 2015-05-27 A. Kawka , S. Vennes , S. O'Toole , P. Nemeth , D. Burton , E. Kotze , D. A. H. Buckley

A chemical abundance analysis is made of two F type high proper motion stars selected from the {\sc ELODIE} library. We use high resolution (R=42\,000) and high signal to noise ratio (S/N=103, 36 $-$per$-$pixel) \'echelle spectra from the…

Solar and Stellar Astrophysics · Physics 2014-09-17 S. Oktay Solakci , Timur Sahin , Christopher Flynn , Ahmet Dervisoglu

Three Galactic O-type stars belong to the rare class of Of?p objects: HD108, HD191612, and HD148937. The first two stars show a wealth of phenomena, including magnetic fields and strong X-ray emission, light variability, and dramatic…

Astrophysics · Physics 2009-11-13 Y. Naze , N. R. Walborn , G. Rauw , F. Martins , A. M. T. Pollock , H. E. Bond

We present adaptive optics JHKs imaging observations of three main-sequence late B-type stars listed in the Lindroos Catalogue: HD123445, HD127971 and HD129791. Given their spectral types, these stars should not be X-ray emitters. However,…

Astrophysics · Physics 2009-11-06 N. Huelamo , W. Brandner , A. G. A. Brown , R. Neuhaeuser , H. Zinnecker

In this paper, we present our HARPS radial-velocity data for eight low-activity solar-type stars belonging to the HARPS volume-limited sample: HD6718, HD8535, HD28254, HD290327, HD43197, HD44219, HD148156, and HD156411. Keplerian fits to…

We report precise Doppler measurements of the stars HD 216437, HD 196050 and HD 160691 obtained with the Anglo-Australian Telescope using the UCLES spectrometer together with an iodine cell as part of the Anglo-Australian Planet Search. Our…

As part of an All-Sky Automated Survey for SuperNovae (ASAS-SN) search for sources with large flux decrements, we discovered a transient where the quiescent, stellar source, ASASSN-V J192114.84+624950.8, rapidly decreased in flux by…

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