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相关论文: Radial Velocity Variations in Pulsating Ap Stars. …

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We present recent results from our radial velocity (RV) studies of rapidly oscillating Ap (roAp) stars. Our measurements reveal that the pulsational amplitude of these stars depends on the spectral region that is examined. For one star,…

天体物理学 · 物理学 2007-05-23 A. P. Hatzes , A. Kanaan

We present detailed analysis of the vertical pulsation mode cross-section in ten rapidly oscillating Ap (roAp) stars based on spectroscopic time-series observations. The aim of this analysis is to derive from observations a complete picture…

天体物理学 · 物理学 2009-11-13 T. Ryabchikova , M. Sachkov , O. Kochukhov , D. Lyashko

Studies based on high-resolution spectroscopic data of rapidly oscillating Ap stars show a surprising diversity of pulsation behavior in the atmospheric layers, pointing, in particular, to the co-existence of running and standing waves. The…

太阳与恒星天体物理 · 物理学 2015-05-27 J. C. Sousa , M Cunha

We present the analysis of spectroscopic time-series observations of the roAp star 10 Aql. Observations were carried out in July 2006 with the UVES and SARG spectrographs simultaneously with the MOST mini-satellite photometry. All these…

天体物理学 · 物理学 2010-11-26 M. Sachkov , O. Kochukhov , T. Ryabchikova , F. Leone , S. Bagnulo , W. W. Weiss

High-resolution spectroscopic time series of rapidly oscillating Ap stars show evidence for a co-existence of standing and running waves in their atmospheric layers. With the purpose of understanding these observations we have carried out a…

天体物理学 · 物理学 2009-06-23 J. C. Sousa , M. S. Cunha

We have investigated the structure of the pulsating atmosphere of one of the best studied rapidly oscillating Ap stars, HD 24712. For this purpose we analyzed spectra collected during 2001-2004. An extensive data set was obtained in 2004…

We have carried out the first survey of the pulsational line profile variability in rapidly oscillating Ap (roAp) stars. We analysed high signal-to-noise time-series observations of ten sharp-lined roAp stars obtained with the…

天体物理学 · 物理学 2008-11-26 O. Kochukhov , T. Ryabchikova , W. W. Weiss , J. D. Landstreet , D. Lyashko

The rapidly oscillating Ap (roAp) star 10 Aql shows one of the lowest photometric pulsation amplitudes and is characterized by an unusual spectroscopic pulsational behavior compared to other roAp stars. More than 1000 spectra were taken…

天体物理学 · 物理学 2009-11-13 M. Sachkov , O. Kochukhov , T. Ryabchikova , D. Huber , F. Leone , S. Bagnulo , W. W. Weiss

We present the analysis of 3 hrs of a rapid time series of precise stellar radial velocity (RV) measurements (sigma = 4.5 m/s) of the cool Ap star Beta CrB. The integrated RV measurements spanning the wavelength interval 5000-6000 Ang. show…

天体物理学 · 物理学 2009-11-10 Artie P. Hatzes , David E. Mkrtichian

Time-resolved spectroscopic observations of rapidly oscillating Ap (roAp) stars show a complex picture of propagating magneto-acoustic pulsation waves, with amplitude and phase strongly changing as a function of atmospheric height. We have…

太阳与恒星天体物理 · 物理学 2015-03-13 O. Kochukhov , E. Khomenko

Over the last decade significant amounts of high-spectral and time-resolution spectroscopic data have been acquired for a number of rapidly oscillating Ap stars. Progress in the understanding of the information held by these data requires…

太阳与恒星天体物理 · 物理学 2018-08-01 Paola Quitral-Manosalva , Margarida S. Cunha , Oleg Kochukhov

We have used high-speed spectroscopy of the rapidly oscillating Ap (roAp) star HD99563 to study the pulsation amplitude and phase behaviour of elements in its stratified atmosphere over one 2.91-d rotation cycle. We identify spectral…

太阳与恒星天体物理 · 物理学 2015-05-13 L. M. Freyhammer , D. W. Kurtz , V. G. Elkin , G. Mathys , I. Savanov , W. Zima , H. Shibahashi , K. Sekiguchi

The rapidly oscillating Ap stars are of importance for studying the atmospheric structure of stars where the process of chemical element diffusion is significant. We have performed a survey for rapid oscillations in a sample of 9 luminous…

天体物理学 · 物理学 2009-11-13 L. M. Freyhammer , D. W. Kurtz , M. S. Cunha , G. Mathys , V. G. Elkin , J. D. Riley

Many types of stars show periodic variations of radius and brightness, which are commonly referred to as `stellar pulsations'. Observed pulsational characteristics are determined by fundamental stellar parameters. Consequently,…

天体物理学 · 物理学 2016-08-30 O. Kochukhov

Three topics are discussed: 1) Photometric observations of the rapidly oscillating Ap stars have shown that the pulsation amplitude drops dramatically as a function of wavelength from the blue to the red. A theoretical derivation, plus…

天体物理学 · 物理学 2007-05-23 D. W. Kurtz

We report the first comprehensive investigation of the line profile variation caused by non-radial pulsation in a magnetic oscillating chemically peculiar star. Spectrum variation of the well-known roAp star HR 3831 is detected using very…

天体物理学 · 物理学 2009-11-11 O. Kochukhov

We present the analysis of K2 short cadence data of the rapidly oscillating Ap (roAp) star, 33 Librae (HD 137949). The precision afforded to the K2 data allow us to identify at least 11 pulsation modes in this star, compared to the three…

太阳与恒星天体物理 · 物理学 2018-08-08 Daniel L. Holdsworth , Margarida S. Cunha , Hiromoto Shibahashi , Donald W. Kurtz , Dominic M. Bowman

We present our discovery of pulsational radial-velocity variations in the cool Ap star HD 75445, an object spectroscopically similar to the bright, rapidly-oscillating Ap (roAp) star gamma Equ. Based on high-resolution time-series…

天体物理学 · 物理学 2009-11-13 O. Kochukhov , S. Bagnulo , G. Lo Curto , T. Ryabchikova

We have carried out a survey of short-period pulsations among a sample of carefully chosen cool Ap stars using time-resolved observations with the UVES spectrometer at the ESO 8-m VLT telescope. Here we report the discovery of pulsations…

太阳与恒星天体物理 · 物理学 2015-06-15 O. Kochukhov , D. Alentiev , T. Ryabchikova , S. Boyko , M. Cunha , V. Tsymbal , W. Weiss

We present results of the radial velocity (RV) analysis of spectroscopic time-series observations of the roAp star HD24712 (HR1217) which were carried out simultaneously with the Canadian MOST mini-satellite photometry. Only lines of the…

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