Zobrazeno 1 - 10
of 25
pro vyhledávání: '"Ai-Ying Zhou"'
Autor:
Min-Yu Li, Sheng-Bang Qian, Ai-Ying Zhou, Li-Ying Zhu, Wen-Ping Liao, Er-Gang Zhao, Xiang-Dong Shi, Fu-Xing Li, Qi-Bin Sun
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 2, p 278 (2024)
Heartbeat stars (HBSs) with tidally excited oscillations (TEOs) are ideal astrophysical laboratories for studying the internal properties of the systems. In this paper, five new HBSs exhibiting TEOs are discovered using TESS photometric data. The orb
Externí odkaz:
https://doaj.org/article/de5c8261c3f34223b93d2cd43a2c93ba
Autor:
Ai-Ying Zhou1 aiying@bao.ac.cn
Publikováno v:
Astrophysics & Space Science. Jan2006, Vol. 301 Issue 1-4, p11-20. 10p. 5 Charts, 8 Graphs.
Autor:
Ai-Ying Zhou1 aiying@bao.ac.cn, Yu-Lei Qiu1
Publikováno v:
Astrophysics & Space Science. 2003, Vol. 288 Issue 3, p327-339. 13p.
Autor:
A. Rolland, J. M. García, P. van Cauteren, Ai-Ying Zhou, P. B. Etzel, F. J. Aceituno, E. Rodriguez, Matt A. Wood, Vlad Turcu, Jadwiga Daszyńska-Daszkiewicz, M. J. Lopez-Gonzalez, Alexandru Pop, D. Díaz-Fraile, David Mkrtichian, Alfredo Sota, Patricia Lampens, Duk-Hang Lee, V. Costa, E. C. Olson, V. Casanova, Dan Moldovan, Pedro J. Amado, Seung-Lee Kim, Eric G. Hintz
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 408:2149-2162
We present the results of a three-continent multisite photometric campaign carried out on the Algol-type eclipsing binary system RZ Cas, in which the primary component has recently been discovered to be a δ Sct-type pulsator. The present observation
Publikováno v:
Research in Astronomy and Astrophysics. 9:349-366
We describe a new BV RI multicolor CCD photometric system situated at the prime focus of the 85-cm telescope at the Xinglong Station of NAOC. Atmospheric extinction effects, photometric accuracy and color calibration dependence of the system are inve
Autor:
Ai-Ying Zhou
Publikováno v:
Chinese Journal of Astronomy and Astrophysics. 4:335-342
Wavelet transform is applied to reanalyze the low amplitude δ Scuti star HD 52788, which exhibits complex light variations with uncertain frequency solutions. We gain an insight into the strong instability of pulsation present in the star. Based on
Autor:
Ai-Ying Zhou
Publikováno v:
Chinese Journal of Astronomy and Astrophysics. 2:43-50
Photometric results of three δ Scuti stars, AD Ari, IP Vir and YZ Boo from new observations obtained at the Xinglong Station of the Beijing Astronomical Observatory(BAO) during 2000 and 2001 are reported. We present here the preliminary analyses. De
Publikováno v:
Chinese Journal of Astronomy and Astrophysics. 2:59-65
UV Tri was observed photometrically from 1999 to 2000 at the Xinglong Station of the National Astronomical Observatories, Chinese Academy of Sciences, and was also observed with Stromgren uvbyH filter system at the Sierra Nevada Observatory (Spain) i
Publikováno v:
Astrophysics and Space Science. 281:699-714
The new time-resolved CCD photometry of XX Cyg was presented. We investigate the time-dependent behaviour of the light variations by reanalyzing the data in the literature. XX Cyg was demonstrated beyond any doubt again to be a monoperiodic pulsator.