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相关论文: Pulsation models for the roAp star HD 134214

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We undertook a time-series photometric multi-site campaign for the rapidly oscillating Ap star HD 99563 and also acquired mean light observations over two seasons. The pulsations of the star, that show flatter light maxima than minima, can…

HR 1217 is a prototypical rapidly oscillating Ap star that has presented a test to the theory of nonradial stellar pulsation. Prior observations showed a clear pattern of five modes with alternating frequency spacings of 33.3 microHz and…

天体物理学 · 物理学 2009-11-07 D. W. Kurtz , S. D. Kawaler , R. L. Riddle et al.

Magnetic perturbations to the frequencies of low degree, high radial order, axisymmetric pulsations in stellar models permeated by large scale magnetic fields are presented. Magnetic fields with dipolar, quadrupolar and a superposition of…

天体物理学 · 物理学 2008-11-26 M. S. Cunha

With FORS1 at the VLT we have tried for the first time to measure the magnetic field variation over the pulsation cycle in six roAp stars to begin the study of how the magnetic field and pulsation interact. For the star HD101065, which has…

天体物理学 · 物理学 2009-11-10 S. Hubrig , D. W. Kurtz , S. Bagnulo , T. Szeifert , M. Schoeller , G. Mathys , W. A. Dziembowski

The large-scale magnetic fields detected at the surface of about 10% of hot stars extend into the stellar interior, where they may alter the structure. Deep inner regions of stars are only observable using asteroseismology. Here, we…

太阳与恒星天体物理 · 物理学 2018-09-05 B. Buysschaert , C. Aerts , D. M. Bowman , C. Johnston , T. Van Reeth , M. G. Pedersen , S. Mathis , C. Neiner

HD 12098 is an roAp star pulsating in the most distorted dipole mode yet observed in this class of star. Using TESS Sector 58 observations we show that there are photometric spots at both the magnetic poles of this star. It pulsates…

太阳与恒星天体物理 · 物理学 2024-02-12 D. W. Kurtz , H. Saio , D. L. Holdsworth , Santosh Joshi , S. Seetha

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 discovery of pulsational variations in the cool magnetic Ap star HD 115226 -- the first high-amplitude rapidly oscillating Ap star discovered with time-series spectroscopy. Using high-resolution spectra obtained with the…

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

The mechanism for excitation of p-modes in rapidly oscillating, peculiar A (roAp, or cool chemically peculiar, CP) stars is unknown. Observations strongly suggest that acoustic modes in roAp stars are causally linked to the stars' magnetic…

天体物理学 · 物理学 2007-05-23 E. J. Zita

We present an analysis of the first Kepler K2 mission observations of a rapidly oscillating Ap (roAp) star, HD 24355 ($V=9.65$). The star was discovered in SuperWASP broadband photometry with a frequency of 224.31 d$^{-1}$, (2596.18…

太阳与恒星天体物理 · 物理学 2016-08-17 Daniel L. Holdsworth , Donald W. Kurtz , Barry Smalley , Hideyuki Saio , Gerald Handler , Simon J. Murphy , Holger Lehmann

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

Rapidly oscillating Ap stars exhibit an astrophysically interesting combination of strong, dipolar-like magnetic fields and high-overtone p-mode pulsations similar to the Sun. Recent time-resolved spectroscopy of these stars unravelled a…

太阳与恒星天体物理 · 物理学 2014-11-20 E. Khomenko , O. Kochukhov

HD 60435 is a well-known rapidly oscillating (roAp) Ap star with a series of alternating even and odd degree modes, making it a prime asteroseismic target. It is also an oblique pulsator with rotational inclination, $i$, and…

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 present high-precision time-series photometry of the classical delta Scuti star HD 144277 obtained with the MOST (Microvariability and Oscillations of STars) satellite in two consecutive years. The observed regular frequency patterns are…

We report the detection of periodic variations on the T_eff ~32 000 K DA white dwarf star HE 1017-1352. We obtained time series photometry using the 4.1 m SOAR telescope on three separate nights for a total of 16.8 h. From the frequency…

太阳与恒星天体物理 · 物理学 2020-06-10 Alejandra D. Romero , L. Antunes Amaral , S. O. Kepler , L. Fraga , D. Kurtz , H. Shibahashi

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

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

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

Using multi-site spectroscopic data collected from three sites, the frequencies and pulsational modes of the {\gamma} Doradus star HD 12901 were identified. A total of six frequencies in the range 1-2 c/d were observed, their…

太阳与恒星天体物理 · 物理学 2015-06-11 E. Brunsden , K. R. Pollard , P. L. Cottrell , D. J. Wright , P. De Cat