Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Kadirya Tursun"'
Autor:
Mengke Zhao, Jianjun Zhou, Willem A. Baan, Yue Hu, A. Lazarian, Xindi Tang, Jarken Esimbek, Yuxin He, Dalei Li, Weiguang Ji, Zhengxue Chang, Kadirya Tursun
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 1, p 18 (2024)
We report the detection of the ordered alignment between the magnetic field and kpc-scale bubbles in the nearby spiral galaxy, NGC 628. Applying the Velocity Gradient Technique on CO spectroscopic data from the ALMA-PHANGS, the magnetic field of NGC
Externí odkaz:
https://doaj.org/article/b8c2f9e280314bcf87b0aa764dc610cd
Autor:
Mengke Zhao, Guang-Xing Li, Jianjun Zhou, Xindi Tang, Jarken Esimbek, Yuxin He, Dalei Li, Weiguang Ji, Zhengxue Chang, Kadirya Tursun
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 1, p 124 (2024)
We study the magnetic field structures in six giant filaments associated with the spiral arms of the Milky Way by applying the velocity gradient technique (VGT) to the ^13 CO spectroscopic data from the GRS, FUGIN, and SEDIGSM surveys. Unlike dust-po
Externí odkaz:
https://doaj.org/article/497f51a7b2294b5aa8313b39fb64332d
Autor:
Mengke Zhao, Jianjun Zhou, Yue Hu, A. Lazarian, Xindi Tang, Willem A. Baan, Jarken Esimbek, Yuxin He, Dalei Li, Weiguang Ji, Kadirya Tursun
Magnetic fields play an important role in the evolution of molecular clouds and star formation. Using the Velocity Gradient Technique (VGT) model, we measured the magnetic field in Orion A using the 12CO, 13CO, and C18O (1-0) emission lines at a scal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e7509b56e227e9ff0e63430adaf573ea
Autor:
T. L. Wilson, Friedrich Wyrowski, A. Malawi, Kadirya Tursun, Gang Wu, Xindi Tang, K. Immer, Rainer Mauersberger, Jianjun Zhou, Jarken Esimbek, E. Alkhuja, H. Asiri, Carsten Henkel
Publikováno v:
Astronomy & Astrophysics, 658:A34
At a distance of 2.4kpc, W33 is an outstanding massive and luminous 10pc sized star forming complex containing quiescent infrared dark clouds as well as highly active infrared bright cloud cores heated by young massive stars. We report measurements o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c210c79f7ade510ca03922d9e4349a9a
Autor:
Xindi Tang, Christian Henkel, Dalei Li, Toktarkhan Komesh, Kadirya Tursun, Gang Wu, Yuxin He, Serikbek Sailanbek, Jarken Esimbek, Jianjun Zhou
Publikováno v:
Astronomy & Astrophysics. 643:A178
We surveyed the Aquila Rift complex including the Serpens South and W 40 regions in the NH3 (1,1) and (2,2) transitions making use of the Nanshan 26-m telescope. Our observations cover an area of ~ 1.5° × 2.2° (11.4 pc × 16.7 pc). The kinetic tem