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相关论文: The Pre-He White Dwarfs in Eclipsing Binaries. I. …

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EL CVn-type systems represent a rare evolutionary stage in binary star evolution, providing ideal laboratories for investigating stable mass transfer processes and the formation of extremely low-mass white dwarfs (ELM WDs). The Transiting…

太阳与恒星天体物理 · 物理学 2024-12-13 Jianping Xiong , Zhenwei Li , Jiao Li , Xiaobin Zhang , Xiaodian Chen , Kaifan Ji , Zhanwen Han , Xuefei Chen

We report the discovery of a relatively bright eclipsing binary system, which consists of a white dwarf and a main sequence K7 star with clear signs of chromospheric and spot activity. The light curve of this system shows $\sim0.2$mag…

EX Hya is one of the few double-lined eclipsing cataclysmic variables that allow an accurate measurement of the binary masses. We analyze orbital phase-resolved UVES/ VLT high resolution spectroscopic observations of EX Hya with the aims of…

天体物理学 · 物理学 2008-02-19 K. Beuermann , K. Reinsch

We report the discovery of a bright (V ~ 13.7), extremely low-mass white dwarf in a close double degenerate system. We originally selected GALEX J171708.5+675712 for spectroscopic follow-up among a group of white dwarf candidates in an…

太阳与恒星天体物理 · 物理学 2011-08-02 S. Vennes , J. R. Thorstensen , A. Kawka , P. Nemeth , J. N. Skinner , A. Pigulski , M. Steslicki , Z. Kolaczkowski , P. Srodka

We report the discovery and characterisation of a new M-dwarf binary, with component masses and radii of M1 = 0.244 -0.003/+0.003 Msun, R1 = 0.261 -0.009/+0.006 Rsun, M2 = 0.179 -0.001/+0.002 Msun, R2 = 0.218 -0.011/+0.007 Rsun, and orbital…

We present high-speed ULTRACAM and SOFI photometry and X-shooter spectroscopy of the recently discovered 94 minute orbital period eclipsing white dwarf / main-sequence binary SDSS J085746.18+034255.3 (CSS 03170) and use these observations…

We have identified a star in the WASP archive photometry with an unusual lightcurve due to the total eclipse of a small, hot star by an apparently normal A-type star and with an orbital period of only 0.668d. From an analysis of the WASP…

We report the discovery and analysis of 36 new eclipsing EL CVn-type binaries, consisting of a core helium-composition pre-white dwarf and an early-type main-sequence companion, more than doubling the known population of these systems. We…

太阳与恒星天体物理 · 物理学 2018-02-14 J. van Roestel , T. Kupfer , R. Ruiz-Carmona , P. J. Groot , T. A. Prince , K. Burdge , R. Laher , D. L. Shupe , E. Bellm

VLT/UVES spectroscopic and TESS photometric observations for WASP 0346-21 allow the direct determination of its physical properties, along with the detection of a circumbinary object and oscillating signals. The high-resolution spectra…

太阳与恒星天体物理 · 物理学 2024-07-26 Jae Woo Lee , Kyeongsoo Hong , Min-Ji Jeong , Marek Wolf

With the prevalence of wide-field, time-domain photometric sky surveys, the number of eclipsing white dwarf systems being discovered is increasing dramatically. An efficient method to follow these up will be key to determining any…

EL CVn-type eclipsing binaries are composed of a massive A-type main-sequence primary star and a hotter B-type secondary star. This paper presents the time-series photometric and asteroseismic results of the EL CVn-type star 1SWASP…

太阳与恒星天体物理 · 物理学 2021-11-03 Seung-Lee Kim , Jae Woo Lee , Chung-Uk Lee , Yongseok Lee , Dong-Joo Lee , Kyeongsoo Hong , Sang-Mok Cha , Dong-Jin Kim , Byeong-Gon Park

We analyze the spectrum of an unusually-low mass white dwarf, SDSSJ123410.37-022802.9 (0335-264-52000), found in our recent, white dwarf catalog from the SDSS DR1 data release. Two independent, model atmosphere fits result in an accurate…

In the past, SDSS J160429.12+100002.2 was spectroscopically classified as a blue horizontal branch (BHB) star. Assuming a luminosity that is characteristic of BHB stars, the object's radial velocity and proper motions from Gaia Early Data…

太阳与恒星天体物理 · 物理学 2021-06-22 Andreas Irrgang , Stephan Geier , Ulrich Heber , Thomas Kupfer , Kareem El-Badry , Steven Bloemen

HW Vir systems are rare evolved eclipsing binaries composed by a hot compact star and a low-mass main-sequence star in a close orbit. These systems provide a direct way to measure the fundamental properties, e.g. masses and radii, of their…

太阳与恒星天体物理 · 物理学 2017-10-25 Leonardo A. Almeida , Augusto Damineli , Cláudia V. Rodrigues , Marildo G. Pereira , Francisco Jablonski

Binaries with a white dwarf primary and a main sequence secondary can be used to test our understanding of both single and binary star evolution. A small fraction of such systems experienced a common-envelope phase from which they emerged…

太阳与恒星天体物理 · 物理学 2022-08-08 R. Priyatikanto , C. Knigge , S. Scaringi , J. Brink , D. A. H. Buckley

We present the first dynamical determination of the binary parameters of an eclipsing SW Sextantis star in the 3-4 hour orbital period range during a low state. We obtained time-resolved optical spectroscopy and photometry of HS 0220+0603…

We present 2271 radial velocity measurements taken on 118 single-line binary stars, taken over eight years with the CORALIE spectrograph. The binaries consist of F/G/K primaries and M-dwarf secondaries. They were initially discovered…

We present the discovery of \thisstar\ (HD 58730), a very low mass ratio ($q \equiv M_2/M_1 \approx 0.07$) eclipsing binary (EB) identified by the Kilodegree Extremely Little Telescope (KELT) survey. We present the discovery light curve and…

We present echelle spectra of TIC 399725538 obtained in Korea and Thailand to investigate the physical properties and evolutionary scenarios of EL CVn-type binaries. The time-series spectra yielded the radial velocities (RVs) of the primary…

太阳与恒星天体物理 · 物理学 2026-01-30 Jae Woo Lee , Kyeongsoo Hong , Min-Ji Jeong , Pakakaew Rittipruk , Jang-Ho Park

We report the discovery of the first eclipsing detached double white dwarf (WD) binary. In a pulsation search, the low-mass helium core WD NLTT 11748 was targeted for fast (approx 1 minute) differential photometry with the Las Cumbres…

太阳与恒星天体物理 · 物理学 2015-05-18 Justin D. R. Steinfadt , David L. Kaplan , Avi Shporer , Lars Bildsten , Steve B. Howell