Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Dongtao Cao"'
Publikováno v:
The Astrophysical Journal, Vol 976, Iss 2, p 217 (2024)
We present a series of nine Doppler images of the magnetically active K component of the RS CVn-type binary SZ Piscium (SZ Psc), based on high-resolution spectroscopic data collected from 2014 to 2018. We apply least-squares deconvolution (LSD) to al
Externí odkaz:
https://doaj.org/article/87780354b409483a8935854d65c1b56e
Autor:
Dongtao Cao, Shenghong Gu
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 1, p 13 (2024)
Stellar coronal mass ejections (CMEs) have recently attracted much attention for their impacts on stellar evolution and surrounding exoplanets. RS CVn-type stars could produce large flares, and therefore may have frequent CMEs. Here we report the cap
Externí odkaz:
https://doaj.org/article/7a7cc534a2704b5cb449ae8400e68009
Autor:
Jianhua Wang, Shenghong Gu, Xiaobin Wang, Bill Yeung, Eric Ng, Kamfung Yu, Leilei Sun, Yue Xiang, Dongtao Cao, Jinming Bai, Yufeng Fan, Fukun Xu, Yisi Liu, Xiaoyun Xu, Nanping Luo
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:6295-6304
We present optimized physical parameters of the active eclipsing binary system USNO-B1.0 1387-0467554 discovered recently in Yunnan–Hong Kong wide-field photometric (YNHK) survey, based on the analysis of its two colour light curves and low resolut
Autor:
Xiaoyun Xu, Xiaobing Wang, Karri Muinonen, Antti Penttilä, Nanping Luo, Shenghong Gu, Leilei Sun, Fukun Xu, Yisi Liu, Yue Xiang, Dongtao Cao, Jianhua Wang
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:3925-3938
The lightcurves of asteroids are essential for determining their physical characteristics, including shape, spin, size, and surface composition. However, most asteroids are missing some of these basic physical parameters due to lack of photometric da
Autor:
Shenghong Gu, Xiaobin Wang, Bill Yeung, Eric Ng, Kamfung Yu, Jinming Bai, Yufeng Fan, Leilei Sun, Yue Xiang, Dongtao Cao, Baoli Lun, Yuxin Xin, Chuanjun Wang, Fukun Xu, Yisi Liu
Publikováno v:
Astronomische Nachrichten. 343
Autor:
Shenghong Gu, Xiaobin Wang, Bill Yeung, Eric Ng, Kamfung Yu, Jinming Bai, Yufeng Fan, Leilei Sun, Yue Xiang, Dongtao Cao, Baoli Lun, Yuxin Xin, Chuanjun Wang, Fukun Xu, Yisi Liu
Publikováno v:
Astronomische Nachrichten. 343
Publikováno v:
Cao, D, Gu, S, Grundahl, F & Palle, P L 2022, ' Magnetic activities on two single-lined RS Canum Venaticorum binaries IM Pegasi and σ Geminorum ', Monthly Notices of the Royal Astronomical Society, vol. 514, no. 3, pp. 4190-4204 . https://doi.org/10.1093/mnras/stac1576
We present the study on continuous high-resolution spectroscopic observations of two long-period single-lined RS Canum Venaticorum (RS CVn) binary stars IM Pegasi (IM Peg) and σ Geminorum (σ Gem), obtained with the Hertzsprung SONG telescope during
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d053c0573db310ff7f9767e4f51bc488
https://pure.au.dk/portal/da/publications/magnetic-activities-on-two-singlelined-rs-canum-venaticorum-binaries-im-pegasi-and--geminorum(c5b0d4c9-d4e6-4cd3-8638-a2b6fdd6b8a8).html
https://pure.au.dk/portal/da/publications/magnetic-activities-on-two-singlelined-rs-canum-venaticorum-binaries-im-pegasi-and--geminorum(c5b0d4c9-d4e6-4cd3-8638-a2b6fdd6b8a8).html
We apply the variational autoencoder (VAE) to the LAMOST-K2 low-resolution spectra to detect the magnetic activity of the stars in the K2 field. After the training on the spectra of the selected inactive stars, the VAE model can efficiently generate
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24101b62c17c4e116cfb38d9597d9780
Autor:
Yisi Liu, Shenghong Gu, Jing Liu, Xiaobin Wang, Bill Yeung, Eric Ng, Jianhua Wang, Yue Xiang, Dongtao Cao, Leilei Sun, Fukun Xu, Xiang Luo, Lu Bai, Xiaoyun Xu
Publikováno v:
The Astronomical Journal. 163:167
USNO-B1.0 1421-0485411 is an eclipsing binary system newly discovered in the Yunnan-Hong Kong wide-field photometric survey. Its orbital period is 1.295 days. Based on the V- and R-band photometric data collected at Kunming 1.0 m telescope and spectr
Autor:
Yimin Ma, Dongtao Cao
Publikováno v:
Journal of Physics: Conference Series. 1802:032123
The three-stage Clos switching network is a kind of multi-stage switching network which is commonly used to build a high-speed and large-capacity switching network, and the scheduling algorithm of the switching network affects the performance of the