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相关论文: HD 34700: A new T Tauri double-lined spectroscopic…

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Monitoring the long-term radial velocity (RV) and acceleration of nearby stars has proven an effective method for directly detecting binary and substellar companions. Some fraction of nearby RV trend systems are expected to be comprised of…

HD49798 / RXJ0648.0-4418 is the only confirmed X-ray binary in which the mass donor is a hot subdwarf star of O spectral type and, most likely, it contains a massive white dwarf (1.28$\pm$0.05 M$_{\rm SUN}$) with a very fast spin period of…

太阳与恒星天体物理 · 物理学 2021-04-21 S. Mereghetti , F. Pintore , T. Rauch , N. La Palombara , P. Esposito , S. Geier , I. Pelisoli , M. Rigoselli , V. Schaffenroth , A. Tiengo

We present the first visible wavelength images of the GG Tauri circumbinary ring, obtained with the Hubble Space Telescope's Wide Field and Planetary Camera 2. Scattered light from the ring is detected in both V and I band images. The…

天体物理学 · 物理学 2009-11-07 J. E. Krist , K. R. Stapelfeldt , A. M. Watson

The emission-line Be star HD 215227 lies within the positional error circle of the newly identified gamma-ray source AGL J2241+4454. We present new blue spectra of the star, and we point out the morphological and variability similarities to…

太阳与恒星天体物理 · 物理学 2015-05-20 S. J. Williams , D. R. Gies , R. A. Matson , Y. Touhami , E. D. Grundstrom , W. Huang , M. V. McSwain

We present the results of a spectroscopic and photometric analysis of HD314884, a slowly pulsating B star (SPB) in a binary system with detected soft X-ray emission. We spectrally classify the B star as a B5V-B6V star with T$_{eff}$ =…

太阳与恒星天体物理 · 物理学 2015-06-22 Christopher B. Johnson , R. I. Hynes , T. Maccarone , C T. Britt , H. Davis , P. G. Jonker , M. A. P. Torres , D. Steeghs , S. Greiss , G. Nelemans

A combination of high-resolution and wide-field imaging reveals two binary stars and one triple star system among the sample of the first 11 stars with planets detected by radial velocity variations. High resolution speckle or adaptive…

We report time-resolved, high-resolution optical spectropolarimetric observations of the young double-lined spectroscopic binary V1878 Ori. Our observations were collected with the ESPaDOnS spectropolarimeter at the Canada-France-Hawaii…

We present observational results from optical long-slit spectroscopy of parsec-scale jets of DG Tau. From HH 158 and HH 702, the optical emission lines of H_alpha, [O I] 6300, 6363, [N II] 6548, 6584, and [S II] 6716, 6731 are obtained. The…

太阳与恒星天体物理 · 物理学 2015-05-20 Heeyoung Oh , Tae-Soo Pyo , In-Soo Yuk , Byeong-Gon Park

Beta Cen is a bright Beta Cephei variable and has long been suspected to be a binary. Here we report interferometric observations with the 3.9-m Anglo-Australian Telescope at a single epoch which show the star to be a binary with components…

天体物理学 · 物理学 2009-10-30 J. G. Robertson , T. R. Bedding , C. Aerts , C. Waelkens , R. G. Marson , J. R. Barton

We present the results from an optical spectroscopic analysis of the massive stars HD 37366 and HD 54662. We find that HD 37366 is a double-lined spectroscopic binary with a period of 31.8187 +/- 0.0004 days, and HD 54662 is also a double…

We report results of VRI photometric monitoring of the T Tauri star plus disk system HH30. We find that HH30 is highly variable over timescales of a few days with Delta V~1.5 mag, Delta I~1.1 mag. Furthermore we find hints of periodicity…

天体物理学 · 物理学 2009-10-31 Kenneth Wood , Scott Wolk , K. Z. Stanek , George Leussis , Keivan Stassun , Michael Wolff , Barbara Whitney

Context. In multiple pre-main-sequence systems the lifetime of circumstellar disks appears to be shorter than around single stars, and the actual dissipation process may depend on the binary parameters of the systems. Aims. We report high…

太阳与恒星天体物理 · 物理学 2017-07-12 Gergely Csépány , Mario van den Ancker , Péter Ábrahám , Rainer Köhler , Wolfgang Brandner , Felix Hormuth , Hector Hiss

We present our final orbit for the late-type spectroscopic binary HD 1. Employed are 553 spectra from 13 years of observations with our robotic STELLA facility and its high-resolution echelle spectrograph SES. Its long-term radial-velocity…

太阳与恒星天体物理 · 物理学 2021-01-13 Klaus G. Strassmeier , Michael Weber

We report on discovery of unique binary system of dIr galaxies which looks like a low surface brightness tidal stream in the halo of another dwarf galaxy. Both the galaxies are detected in the HI line with the Giant Metrewave Radio…

宇宙学与河外天体物理 · 物理学 2013-03-12 D. Makarov , I. D. Karachentsev , J. N. Chengalur , R. Uklein , A. Marchuk

We report the results of XMM-Newton observations of HD49798/RXJ0648.0-4418, the only known X-ray binary consisting of a hot sub-dwarf and a white dwarf. The white dwarf rotates very rapidly (P=13.2 s) and has a dynamically measured mass of…

高能天体物理现象 · 物理学 2015-05-28 S. Mereghetti , N. La Palombara , A. Tiengo , F. Pizzolato , P. Esposito , P. A. Woudt , G. L. Israel , L. Stella

HD 16429 A is a triple star system consisting of a single-lined spectroscopic binary and a widely separated third component, previously identified via speckle interferometry. Here I present the first orbital elements for the unblended…

天体物理学 · 物理学 2009-11-07 M. V. McSwain

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

Hubble Space Telescope Advanced Camera for Surveys images of the young binary GG Tauri and its circumbinary disk in V and I bandpasses were obtained in 2002 and are the most detailed of this system to date. The confirm features previously…

We started a program to search for companions around hybrid $\delta$ Sct/$\gamma$ Dor stars with the frequency modulation method using Kepler data. Our best candidate was KIC 5709664, where we could identify Fourier peaks with sidelobes,…

New diffraction-limited speckle images of the Red Rectangle in the wavelength range 2.1--3.3 microns with angular resolutions of 44--68 mas and previous speckle images at 0.7--2.2 microns revealed well-resolved bright bipolar outflow lobes…

天体物理学 · 物理学 2009-11-07 Alexander B. Men'shchikov , Dieter Schertl , Peter Tuthill , Gerd Weigelt , Lev R. Yungelson