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Using MOST (Microvariability and Oscillations of STars) satellite guide star photometry, we have discovered a metallic A star showing hybrid p- and g-mode pulsations. HD 114839 was observed nearly continuously for 10 days in March, 2005. We…

Gamma Doradus stars are excellent targets for asteroseismology since the gravity modes present in these stars probe the deep stellar interiors. Mode identification will improve the knowledge of these stars considerably. A selected group of…

Pulsations in pre-main sequence stars have been discovered several times within the last years. But nearly all of these pulsators are of delta Scuti-type. gamma Doradus-type pulsation in young stars has been predicted by theory, but lack…

Solar and Stellar Astrophysics · Physics 2015-06-12 K. Zwintz , L. Fossati , T. Ryabchikova , A. Kaiser , M. Gruberbauer , T. G. Barnes , A. Baglin , S. Chaintreuil

We analyse TESS light curves for 70 southern $\lambda$ Boo stars to identify binaries and to determine which of them pulsate as $\delta$ Scuti stars. We find two heartbeat stars and two eclipsing binaries among the sample. We calculate that…

Solar and Stellar Astrophysics · Physics 2020-05-20 S. J. Murphy , E. Paunzen , T. R. Bedding , P. Walczak , D. Huber

The chemically peculiar (CP) stars HD 98851 and HD 102480 have been discovered to be unusual pulsators during the ``Naini Tal Cape Survey'' programme to search for pulsational variability in CP stars. Time series photometric and…

Astrophysics · Physics 2009-11-07 Santosh Joshi , V. Girish , R. Sagar , D. W. Kurtz , P. Martinez , B. Kumar , S. Seetha , B. N. Ashoka , A. Zhou

Context: We present the results of an extensive ground-based photometric and spectroscopic campaign on the gamma Dor CoRoT target HD49434. This campaign was preparatory to the CoRoT satellite observations, which took place from October 2007…

We have analysed the photometric data obtained with the STEREO spacecraft for 558 non-magnetic chemically peculiar (CP) stars to search for rotational and pulsational variability. Applying the Lomb-Scargle and the phase dispersion…

Solar and Stellar Astrophysics · Physics 2015-06-12 E. Paunzen , K. T. Wraight , L. Fossati , M. Netopil , G. J. White , D. Bewsher

Based on 2-minute cadence TESS data, we investigate pulsations of TIC 65138566 and TIC 139729335 and discover them to be two new HADS stars with equally spaced g modes. We recognize the radial fundamental mode $f_1$ = 18.3334 c/d and the…

Solar and Stellar Astrophysics · Physics 2024-01-25 Xinghao Chen , Xiaobin Zhang , Yan Li , Jie Su

Low frequency oscillation, typical for Gamma Doradus g-mode type stellar core sensitive pulsation, as well as higher frequency Delta Scuti type pulsation typical for p-modes, sensitive to the envelope, make HD 8801 a remarkable hybrid…

Solar and Stellar Astrophysics · Physics 2013-07-15 R. Neuteufel , W. Weiss , G. Handler

We present the mode identification of frequencies found in spectroscopic observations of the Gamma Doradus star HD135825. Four frequencies were successfully identified: 1.3150 +/- 0.0003 1/d; 0.2902 +/- 0.0004 1/d; 1.4045 +/- 0.0005 1/d;…

Solar and Stellar Astrophysics · Physics 2015-06-04 E. Brunsden , K. R. Pollard , P. L. Cottrell , D. J. Wright , P. De Cat , P. M. Kilmartin

We have analysed the chemical photospheric composition of 24 Herbig Ae/Be and Vega-type stars in search for the lambda Bootis phenomenon. We present the results of the elemental abundances of the sample stars. Some of the stars were never…

Astrophysics · Physics 2009-11-10 Bram Acke , Christoffel Waelkens

HD4539 (alias PG0044+097 or EPIC220641886) is a bright (V=10.2) long-period V1093 Her-type subdwarf B (sdB) pulsating star that was observed by the Kepler spacecraft in its secondary (K2) mission. We use the K2 light curve (78.7 days) to…

Solar and Stellar Astrophysics · Physics 2019-08-21 R. Silvotti , M. Uzundag , A. S. Baran , R. H. Ostensen , J. H. Telting , U. Heber , M. D. Reed , M. Vuckovic

[Context.] The hot subdwarf B star HS0702+6043 is known as a large-amplitude, short-period p-mode pulsator of the EC14026 type. Its atmospheric parameters place it at the common boundary between the empirical instability regions of the…

Astrophysics · Physics 2009-11-11 S. Schuh , J. Huber , S. Dreizler , U. Heber , S. J. O'Toole , E. M. Green , G. Fontaine

The Kepler spacecraft is providing photometric time series with micro-magnitude precision for thousands of variable stars. The continuous time-series of unprecedented time span open up opportunities to study the pulsational variability in…

Solar and Stellar Astrophysics · Physics 2011-11-08 K. Uytterhoeven , KASC WG#10

CoRoT ID 105733033 is an excellent example of hybrid pulsators as it shows g- and p-modes with almost similar amplitudes in two clearly distinct frequency domains. Classical Fourier analysis allows the dectection of frequencies with an…

Solar and Stellar Astrophysics · Physics 2015-06-04 E. Chapellier , P. Mathias , W. W. Weiss , D. Le Contel , J. Debosscher

According to most literature sources, the amplitude of the pulsational variability observed in gamma Doradus stars does not exceed 0.1 mag in Johnson V. We have analyzed fifteen high-amplitude gamma Doradus stars with photometric…

Solar and Stellar Astrophysics · Physics 2020-10-22 Ernst Paunzen , Klaus Bernhard , Stefan Huemmerich , Franz-Josef Hambsch , Christopher Lloyd , Sebastian Otero

Based on the LAMOST spectroscopy and TESS time-series photometry, we have obtained a main-sequence star sample of $\delta$ Scuti and $\gamma$ Doradus stars. The sample includes 1534 $\delta$ Sct stars, 367 $\gamma$ Dor stars, 1703 $\delta$…

Solar and Stellar Astrophysics · Physics 2024-11-15 Jiyu Wang , Xiaodian Chen , Licai Deng , Jianxing Zhang , Weijia Sun

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 present the first results of a 2-year high-resolution spectroscopy campaign of 59 candidate Gamma Doradus stars which were mainly discovered from the HIPPARCOS astrometric mission. More than 60 % of the stars present line profile…