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Related papers: High-degree gravity modes in the single sdB star H…

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A spectroscopic analysis of SDSS J160043.6+074802.9, a binary system containing a pulsating subdwarf-O (sdO) star with a late-type companion, yields Teff = 70 000 +/- 5000 K and log g = 5.25 +/- 0.30, together with a most likely type of K3V…

Solar and Stellar Astrophysics · Physics 2015-05-14 C. Rodríguez-López , A. E. Lynas-Gray , D. Kilkenny , J. MacDonald , A. Moya , C. Koen , P. A. Woudt , D. J. Wium , B. Oruru , E. Zietsman

Accurate and extensive photoelectric photometry has been obtained of V994 Her which was discovered as an eclipsing binary by Hipparcos satellite. A marked pulsation activity is evident in the light-curve, with periods 0.152100488,…

Astrophysics · Physics 2007-05-23 S. Dallaporta , U. Munari

We present results on the second-faintest pulsating subdwarf B (sdB) star known, RAT J0455+1305, derived from photometric data obtained in 2009. It shows both short and long periods oscillations, theoretically assigned as pressure and…

Solar and Stellar Astrophysics · Physics 2015-05-27 A. S. Baran , J. T. Gilker , L. Fox-Machado , M. D. Reed , S. D. Kawaler

We propose that KIC 1573174 is a quadruple-mode $\delta$ Scuti star with pulsation amplitudes between those of the HADS (high-amplitude Delta Scuti star) group and average low-amplitude pulsators. The radial modes detected in this star…

Solar and Stellar Astrophysics · Physics 2022-06-22 Chenglong Lv , Ali Esamdin , Javier Pascual-Granado , Taozhi Yang , Dongxiang Shen

We present results of the multicolour UBVR photometry of the high-amplitude EC14026-type star, Balloon 090100001. The data span over a month and consist of more than a hundred hours of observations. Fourier analysis of these data led us to…

Astrophysics · Physics 2009-11-10 A. Baran , A. Pigulski , D. Koziel , W. Ogloza , R. Silvotti , S. Zola

We report on the analysis of high-precision space-based photometry of the roAp (rapidly oscillating Ap) stars HD 9289, HD 99563, and HD134214. All three stars were observed by the MOST satellite for more than 25 days, allowing unprecedented…

Several studies have shown that a number of stars pulsating in p modes lie between the $\beta$ Cep and $\delta$ Sct instability strips in the Hertzsprung-Russell (HR) Diagram. At present, there is no certain understanding of how p~modes can…

Solar and Stellar Astrophysics · Physics 2023-03-29 D. W. Kurtz , R. Jayaraman , P. Sowicka , G. Handler , H. Saio , J. Labadie-Bartz , U. Lee

We report the detection of a substellar companion orbiting an evolved intermediate-mass ($M_\star=2.4\,M_\odot$) star HD 14067 (G9 III) using precise Doppler technique. Radial velocities of this star can be well fitted either by a periodic…

We report the discovery of a 16th magnitude star, HE0437-5439, with a heliocentric radial velocity of +723+-3km/s. A quantitative spectral analysis of high-resolution optical spectra obtained with the VLT and the UVES spectrograph shows…

Astrophysics · Physics 2009-11-13 Heinz Edelmann , Ralf Napiwotzki , Uli Heber , Norbert Christlieb , Dieter Reimers

We investigated the pulsating behavior of KIC 10855535 using Kepler 4-year long cadence data. Two independent frequencies were detected: a pulsation frequency F0 = 17.733260(5)d-1 and a low frequency f8=0.412643(8)d-1 We identify F0 as the…

Solar and Stellar Astrophysics · Physics 2024-11-05 Lixian Shen , Ali Esamdin , Chenglong Lv , Haozhi Wang , Taozhi Yang , Rivkat Karimov , Shuhrat A. Ehgamberdiev , Hubiao Niu , Jinzhong Liu

We report a spectroscopic orbit with period P = 3.52433 +/- 0.00027 days for the planetary companion that transits the solar-type star HD209458. For the metallicity, mass, and radius of the star we derive [Fe/H] = 0.00 +/- 0.02, M = 1.1 +/-…

We report the detection of nonradial g-mode oscillations in the DA white dwarfs HS1039+4112 (B=15.9) and HE1429-0343 (B=15.8) from time-series photometry made at the Loiano 1.5 m telescope. The two stars were previously selected as probable…

Astrophysics · Physics 2007-05-23 R. Silvotti , B. Voss , I. Bruni , D. Koester , D. Reimers , R. Napiwotzki , D. Homeier

The sdB star KPD 0422+5421 was discovered to be a single-lined spectroscopic binary with a period of P=0.0901795 +/- (3\times 10^{-7}) days (2 hours, 10 minutes). The U and B light curves display an ellipsoidal modulation with amplitudes of…

Astrophysics · Physics 2009-10-30 C. Koen , Jerome A. Orosz , Richard A. Wade

The A/F-type stars and pulsators ($\delta$ Scuti-$\gamma$ Dor) are in a critical regime where they experience the transition from radiative to convective transport of energy in their envelopes. Such stars can pulsate in both gravity and…

Solar and Stellar Astrophysics · Physics 2017-12-01 Anya , Samadi Gh. , Patricia Lampens , Davood M. Jassur

Four members of the new class of pulsating sdB stars are analysed from Keck HIRES spectra using NLTE and LTE model atmospheres. Atmospheric parameters (Teff, log g, log(He/H)), metal abundances and rotational velocities are determined.…

Astrophysics · Physics 2018-03-14 U. Heber , I. N. Reid , K. Werner

Pulsed X-ray emission in the luminous, helium-rich sdO BD+37 442 has recently been discovered (La Palombara et al., 2012). It was suggested that the sdO star has a neutron star or white dwarf companion with a spin period of 19.2 s. After HD…

Solar and Stellar Astrophysics · Physics 2014-04-29 U. Heber , S. Geier , A. Irrgang , D. Schneider , I. Barbu-Barna , S. Mereghetti , N. La Palombara

The pulsating DA white dwarfs (ZZ Ceti stars) are $g$-mode non-radial pulsators. Asteroseismology provides strong constraints on their global parameters and internal structure. Since all the DA white dwarfs falling in the ZZ Ceti…

The K2.5 dwarf HD 40307 has been reported to host three super-Earths. The system lacks massive planets and is therefore a potential candidate for having additional low-mass planetary companions. We re-derive Doppler measurements from public…

We have discovered both intermediate-order gravity mode and low-order pressure mode pulsation in the same star, HD 209295. It is therefore both a Gamma Doradus and a Delta Scuti star, which makes it the first pulsating star to be a member…

We present analysis of a new pulsating helium-atmosphere (DB) white dwarf, EPIC~228782059, discovered from 55.1~days of {\em K2} photometry. The long duration, high quality light curves reveal 11 independent dipole and quadruple modes, from…

Solar and Stellar Astrophysics · Physics 2021-11-24 R. M. Duan , W. Zong , J. -N. Fu , Y. H. Chen , J. J. Hermes , Zachary P. Vanderbosch , X. Y. Ma , S. Charpinet
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