English
Related papers

Related papers: Multi-wavelength photometric variation of PG1605+0…

200 papers

We present the results obtained with the CoRoT satellite for HD 50870, a Delta Sct star which was observed for 114.4 d. The 307,570 CoRoT datapoints were analysed with different techniques. The photometric observations were complemented…

In $\delta$ Scuti star models, the photometric amplitudes and phases exhibit a strong dependence on convection, which enters through the complex parameter, $f$, which describes the bolometric flux variation. We present a new method of…

Astrophysics · Physics 2007-05-23 J. Daszy{ń}ska-Daszkiewicz , W. A. Dziembowski , A. A. Pamyatnykh

We collected a sample of ten hitherto unidentified SPB stars with the aim of describing their pulsational properties and identifying pulsational modes. Photometric time series data from various surveys were collected and analyzed using…

Solar and Stellar Astrophysics · Physics 2020-01-22 M. Fedurco , E. Paunzen , S. Hümmerich , K. Bernhard , Š. Parimucha

We present a preliminary analysis of time series photometry on the pulsating subdwarf B star PG1336-018 acquired as part of two Whole Earth Telescope runs. PG1336-018 is a multi-mode pulsator with at least 15 periods centered around 175…

Multicolor photometric data are presented for the CALSPEC stars P177D and P330E. Together with previously published photometry for nine other CALSPEC standards, the photometric observations and synthetic photometry from HST/STIS…

Instrumentation and Methods for Astrophysics · Physics 2015-06-23 Ralph C. Bohlin , Arlo U. Landolt

S5 0716+714 is a well-studied BL Lac object in the sky. Verifying the existence of correlations among the flux variations in different bands serves as an important tool to investigate the emission processes. To examine the possible…

High Energy Astrophysical Phenomena · Physics 2015-05-18 Bingkai Zhang , Benzhong Dai , Li Zhang , Jiali Liu , Zhen Cao

We present a comprehensive multiwavelength analysis of the hot DB white dwarf PG 0112+104. Our analysis relies on newly-acquired FUSE observations, on medium-resolution FOS and GHRS data, on archival high-resolution GHRS observations, on…

Solar and Stellar Astrophysics · Physics 2015-05-19 P. Dufour , S. Desharnais , F. Wesemael , P. Chayer , T. Lanz , P. Bergeron , G. Fontaine , A. Beauchamp , R. A. Saffer , J. W. Kruk , M. -M. Limoges

In order to study short timescale optical variability of $\gamma$-ray blazar S5 0716+714, quasi-simultaneous spectroscopic and multi-band photometric observations were performed from 2018 November to 2019 March with the 2.4 m optical…

Astrophysics of Galaxies · Physics 2021-01-01 Hai-Cheng. Feng , H. T. Liu , J. M. Bai , L. F. Xing , Y. B. Li , M. Xiao , Y. X. Xin

GW Vir variables are the pulsating members in the spectroscopic class of PG 1159 stars. In order to understand the characteristic differences between pulsating and non-pulsating PG 1159 stars, we analyse FUSE spectra of eleven objects, of…

Astrophysics · Physics 2007-05-23 E. Reiff , D. Jahn , T. Rauch , K. Werner , J. W. Kruk , F. Herwig

We have spectroscopically monitored the galactic Luminous Blue Variable HD 160529 and obtained an extensive high-resolution data set that covers the years 1991 to 2002. During this period, the star evolved from an extended photometric…

We report the discovery of a new slowly pulsating B (SPB) star, with the largest number of detected frequencies to date by more than a factor of three, based on 37 days of MOST (Microvariability & Oscillations of STars) satellite guide star…

We continuously monitored the blazar S5 0716+714 in the optical $g$, $r$ and $i$ bands from Nov. 10, 2017 to Jun. 06, 2019. The total number of observations is 201 nights including 26973 data points. This is a very large quasi-simultaneous…

High Energy Astrophysical Phenomena · Physics 2020-04-01 Dingrong Xiong , Jinming Bai , Junhui Fan , Dahai Yan , Minfeng Gu , Xuliang Fan , Jirong Mao , Nan Ding , Rui Xue , Weimin Yi

We review the nature of the oscillations of main-sequence and supergiant stars of spectral type B. Seismic tuning of the interior structure parameters of the $\beta $Cep stars has been achieved since three years. The results are based on…

Astrophysics · Physics 2007-05-23 C. Aerts

While delta Scuti stars are the most numerous class of kappa-mechanism pulsators in the instability strip, the short periods and small peak-to-peak amplitudes have left them understudied and underutilized. Recently, large-scale time-domain…

The subdwarf B (sdB) star V391 Peg oscillates in short-period p modes and long-period g modes, making it one of the three known hybrids among sdBs. As a by-product of the effort to measure secular period changes in the p modes due to…

Solar and Stellar Astrophysics · Physics 2015-05-13 S. Schuh , R. Kruspe , R. Lutz , R. Silvotti

The potential of photometric methods for the identification of l, the degree of spherical surface harmonic of a pulsating star, is investigated with special emphasis on Stromgren photometry applied to delta Scuti and gamma Dor variables.…

Astrophysics · Physics 2007-05-23 Rafael Garrido

The radio and gamma-ray pulsar PSR J2032+4127 was recently found to be in a decades-long orbit with the Be star MT91 213, with the pulsar moving rapidly towards periastron. This binary shares many similar characteristics with the previously…

Solar and Stellar Astrophysics · Physics 2016-10-26 Wynn C. G. Ho , C. -Y. Ng , Andrew G. Lyne , Ben W. Stappers , Malcolm J. Coe , Jules P. Halpern , Tyrel J. Johnson , Iain A. Steele

We present photometric and spectroscopic follow-up observations of short-period variables discovered in the OmegaWhite survey: a wide-field high-cadence g-band synoptic survey targeting the Galactic Plane. We have used fast photometry on…

We report on a multi-site photometric campaign on the high-amplitude $\delta$ Scuti star V2367 Cyg in order to determine the pulsation modes. We also used high-dispersion spectroscopy to estimate the stellar parameters and projected…

We present simultaneous, multi-colour optical light curves of the companion star to the black-widow pulsar PSR J2051-0827, obtained approximately 10 years apart using ULTRACAM and HiPERCAM, respectively. The ULTRACAM light curves confirm…

‹ Prev 1 3 4 5 6 7 10 Next ›