Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Ma, Yingxiu"'
Autor:
Zhang, WenJun, Zhou, Jianjun, Esimbek, Jarken, Baan, Willem, He, Yuxin, Tang, Xindi, Li, Dalei, Ji, Weiguang, Wu, Gang, Ma, Yingxiu, Li, Jiasheng, Zhou, Dongdong, Tursun, Kadirya, Komesh, Toktarkhan
Publikováno v:
A&A 688, A99 (2024)
W49A is a prominent giant molecular cloud (GMC) that exhibits strong star formation activities, yet its structural and kinematic properties remain uncertain. Our study aims to investigate the large-scale structure and kinematics of W49A, and elucidat
Externí odkaz:
http://arxiv.org/abs/2406.08906
Autor:
Ma, Yingxiu, Zhou, Jianjun, Esimbek, Jarken, Baan, Willem, Li, Dalei, Tang, Xindi, He, Yuxin, Ji, Weiguang, Zhou, Dongdong, Wu, Gang, Tursun, Kadirya, Komesh, Toktarkhan
Publikováno v:
A&A 676, A15 (2023)
We studied the hub filament system G323.46-0.08 based on archival molecular line data from the SEDIGISM 13CO survey and infrared data from the GLIMPSE, MIPS, and Hi-GAL surveys. G323.46-0.08 consists of three filaments, F-north, F-west, and F-south,
Externí odkaz:
http://arxiv.org/abs/2306.16875
Autor:
Ma, Yingxiu., Zhou, Jianjun., Esimbek, Jarken., Baan, Willem., Li, Dalei., He, Yuxin., Tang, Xindi., Ji, Weiguang., Zhou, Dongdong., Wu, Gang., Xu, Ye.
Publikováno v:
A&A 663, A97 (2022)
We studied the cloud-cloud collision candidate G323.18+0.15 based on signatures of induced filaments, clumps, and star formation. We used archival molecular spectrum line data from the SEDIGISM $^{13}$CO($J$\,=\,2--1) survey, from the Mopra southern
Externí odkaz:
http://arxiv.org/abs/2205.12624
Publikováno v:
In Journal of Archaeological Science: Reports April 2024 54
Akademický článek
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Autor:
Li, Xu, Esimbek, Jarken, Zhou, Jianjun, Baan, W. A., Ji, Weiguang, Tang, Xindi, Wu, Gang, Tang, Xiaoke, Li, Qiang, Ma, Yingxiu, Sailanbek, Serikbek, Li, Dalei, Alimbetova, Dina
A multi-wavelength analysis of the large Galactic infrared bubble N 24 is has been presented in this paper in order to investigate the molecular and star formation environment around expanding HII regions. Using archival data from Herschel and ATLASG
Externí odkaz:
http://arxiv.org/abs/1905.03565
We performed a detailed study of the high-mass clump interacting with bubble N10 based on the spectral lines $^{12}CO(3-2)$, $HCO^+(4-3)$, $N_2H^+(4-3)$ and $CH_3OH(7(0,7)-6(0,6))$ and continuum emission data at 450 $\mu$m and 850 $\mu$m released on
Externí odkaz:
http://arxiv.org/abs/1303.4914
Autor:
Jiang D; Center for Reproductive Medicine, Department of Obstetrics and Gynecology, Qilu Hospital of Shandong University, Jinan, 250012, PR China., Yang Y; Center for Reproductive Medicine, Department of Obstetrics and Gynecology, Qilu Hospital of Shandong University, Jinan, 250012, PR China., Han X; Center for Reproductive Medicine, Department of Obstetrics and Gynecology, Qilu Hospital of Shandong University, Jinan, 250012, PR China., Li Q; Center for Reproductive Medicine, Department of Obstetrics and Gynecology, Qilu Hospital of Shandong University, Jinan, 250012, PR China., Jiao J; Center for Reproductive Medicine, Department of Obstetrics and Gynecology, Qilu Hospital of Shandong University, Jinan, 250012, PR China., Ma Y; Center for Reproductive Medicine, Department of Obstetrics and Gynecology, Qilu Hospital of Shandong University, Jinan, 250012, PR China., Chao L; Center for Reproductive Medicine, Department of Obstetrics and Gynecology, Qilu Hospital of Shandong University, Jinan, 250012, PR China. Electronic address: chaolan@email.sdu.edu.cn.
Publikováno v:
Environmental pollution (Barking, Essex : 1987) [Environ Pollut] 2024 Nov 18, pp. 125339. Date of Electronic Publication: 2024 Nov 18.