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相关论文: Radial Velocities of Six OB Stars

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We report on new radial velocity measurements of massive stars that are either suspected binaries or lacking prior observations. This is part of a survey to identify and characterize spectroscopic binaries among O-type stars with the goal…

太阳与恒星天体物理 · 物理学 2015-06-11 S. J. Williams , D. R. Gies , T. C. Hillwig , M. V. McSwain , W. Huang

Here we publish the second list of radial velocities for 91 Hipparcos stars, mostly high transverse velocity binaries without previous radial velocity measurements. The measurements of radial velocities are done with a CORAVEL-type radial…

天体物理学 · 物理学 2007-05-23 A. Bartkevicius , J. Sperauskas

Radial-velocity measurements and sine-curve fits to the orbital velocity variations are presented for the fourth set of ten close binary systems: 44 Boo, FI Boo, V2150 Cyg, V899 Her, EX Leo, VZ Lib, SW Lyn, V2377 Oph, Anon Psc (GSC 8-324),…

天体物理学 · 物理学 2009-11-06 W. Lu , S. M. Rucinski , Waldemar Ogloza

We report on the current status of the radial velocity monitoring of nearby OB stars to look for binaries with small mass ratios. The combined data of radial velocities using the domestic 1-2 m-class telescopes seems to confirm the…

太阳与恒星天体物理 · 物理学 2018-12-18 Yuki Moritani , Takuma Suda , Toshikazu Shigeyama , Takayuki R. Saitoh

We derive single-epoch radial velocities for a sample of 56 B-type stars members of the subgroups Upper Scorpius, Upper Centaurus Lupus and Lower Centaurus Crux of the nearby Sco-Cen OB association. The radial velocity measurements were…

天体物理学 · 物理学 2009-11-11 E. Jilinski , S. Daflon , K. Cunha , R. de la Reza

We present new radial velocity measurements of 13 selected intermediate mass stars (2 - 6 M$_\odot$). The measurements were performed between 29 April and 6 September 2024 at the University Observatory Jena using the \'echelle spectrograph…

太阳与恒星天体物理 · 物理学 2025-10-14 J. Bätz , M. Mugrauer , K. -U. Michel , J. Reichert , A. Tschirschky , L. Pietsch , F. Edelmann , R. Neuhäuser

We present the first results of a radial-velocity survey of cool Ap and Am stars. HD 8441 is not only a double system with P = 106.357 days, but is a triple one, the third companion having an orbital period larger than 5000 days. Improved…

天体物理学 · 物理学 2009-10-30 P. North , J. -M. Carquillat , N. Ginestet , F. Carrier , S. Udry

Radial velocity curves for 15 bright subdwarf B binary systems have been measured using high precision radial velocity measurements from high S/N optical high-resolution spectra. In addition, two bright sdB stars are discovered to be radial…

天体物理学 · 物理学 2009-11-11 H. Edelmann , U. Heber , M. Altmann , C. Karl , T. Lisker

We present spectroscopic orbits for the active stars HD 82159 (GS Leo), HD 89959, BD +39 2587 (a visual companion to HD 112733), HD 138157 (OX Ser), HD 143705, and HD 160934. This paper is a sequel to one published in this journal in 2006,…

太阳与恒星天体物理 · 物理学 2015-05-18 R. F. Griffin , N. Filiz Ak

It was recently claimed that the magnetic O-type star HD 54879 exhibits important radial velocity variability indicative of its presence in a spectroscopic binary. More remarkably, it was furthermore reported that the star underwent a…

太阳与恒星天体物理 · 物理学 2020-01-08 G. A. Wade , S. Bagnulo , Z. Keszthelyi , C. P. Folsom , E. Alecian , N. Castro , A. David-Uraz , L. Fossati , V. Petit , M. E. Shultz , J. Sikora

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…

We present the very first analysis of the spectroscopic variability of the three rapidly rotating Oef stars HD192281 (O5(ef)), HD14442 (O5.5ef) and HD14434 (O6.5(ef)). Radial velocities of the HeII lambda 4541 line reveal no evidence of…

天体物理学 · 物理学 2009-11-10 M. De Becker , G. Rauw

Analyses of multi-epoch, high-resolution (~ 50000) optical spectra of seven early-type systems provided various important new insights with respect to their multiplicity. First determinations of orbital periods were made for HD 92206C…

Radial-velocity measurements and sine-curve fits to the orbital velocity variations are presented for nine contact binaries, V1464 Aql, V759 Cen, DE Oct, MW Pav, BQ Phe, EL Aqr, SX Crv, VZ Lib, GR Vir; for the first five among these, our…

天体物理学 · 物理学 2009-11-11 Slavek M. Rucinski , Hilmar Duerbeck

We present the results of time-resolved spectroscopy of 13 O-type stars in the Cas OB6 stellar association. We conducted a survey for radial velocity variability in search of binary systems, which are expected to be plentiful in young OB…

We present the results of a long-term monitoring campaign of the H\alpha line in a sample of bright OB-supergiants (O7.5-B9) that aims at detecting rotationally modulated changes potentially related to the existence of large-scale wind…

天体物理学 · 物理学 2009-11-10 T. Morel , S. V. Marchenko , A. K. Pati , K. Kuppuswamy , M. T. Carini , E. Wood , R. Zimmerman

Radial velocity measurements and simple sine-curve fits to the orbital velocity variations are presented for the second set of ten contact binary systems. Eight systems are of the A-type: AH Aur, CK Boo, DK Cyg, UZ Leo, XZ Leo, V839 Oph, GR…

天体物理学 · 物理学 2009-10-31 Slavek M. Rucinski , Wenxian Lu

In a well-aimed search based on the recently published Gaia~DR2 radial velocity data and performed with the robotic TIGRE telescope, we have discovered 19 bright ($m_V<7.66$~mag) spectroscopic binary stars. We present the radial velocity…

太阳与恒星天体物理 · 物理学 2020-10-07 Dennis Jack , Missael Alejandro Hernández Huerta , Klaus-Peter Schröder

The three objects have been identified as members of the recently recognized class of Gamma Doradus stars, which exhibit multi-periodic photometric variations that are thought to arise from non-radial pulsation. The particular objects…

天体物理学 · 物理学 2007-05-23 R. F. Griffin , H. M. J. Boffin

The star HD 219542 B has been reported by us (Desidera et al. 2003) to show low-amplitude radial velocity variations that could be due to the presence of a Saturn-mass planetary companion or to stellar activity phenomena. In this letter we…

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