Zobrazeno 1 - 10
of 393
pro vyhledávání: '"R. S. Peng"'
Publikováno v:
European Urology Supplements. 16:e931-e932
Autor:
H.J. Chung, A.T.L. Lin, Y.H. Fan, Kuang-Kuo Chen, R.-S. Peng, E.Y-H. Huang, C-C. Lin, Y-H. Chang
Publikováno v:
European Urology Supplements. 15:e871
Autor:
Yu Sun1, Chaofan Li2 CfLi_HEBPU@163.com, Hongcheng Gao1, Jiaming Li1, Jiabin Hao1 jiajooy@163.com
Publikováno v:
Bulletin of the Chemical Society of Ethiopia. 2024, Vol. 38 Issue 5, p1429-1437. 9p.
Autor:
Bakhashab, Sherin1,2,3 (AUTHOR) josieoneill@virginmedia.com, Barber, Rosie2,4 (AUTHOR) catherine.arden@newcastle.ac.uk, O'Neill, Josie2,4 (AUTHOR), Arden, Catherine4 (AUTHOR), Weaver, Jolanta U.2,5,6 (AUTHOR) jolanta.weaver@newcastle.ac.uk
Publikováno v:
International Journal of Molecular Sciences. Aug2024, Vol. 25 Issue 15, p8087. 20p.
Autor:
R. S. Peng, John B. Whiteoak
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 260:529-536
To investigate the observed absorption of the 2 0 →3 −1 E transition of CH 3 OH at 12.2 MHz against the 2.7-K microwave background, statistical equilibrium calculations involving radiative transitions, collisional transitions, and photon trapping
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 260:425-436
We have searched for 12-GHz methanol maser emission from the direction of 173 OH masers in star formation regions and obtained 53 detections, including 19 previously unreported. The observations of these and four other southern methanol masers are pr
Autor:
R. S. Peng, John B. Whiteoak
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 254:301-305
58 southern molecular clouds were searched for CH 3 OH absorption at 12.2 GHz, yielding 38 detections. The absorption has a median brightness temperature of 0.22 K, linewidth of 4.2 km/s, and velocity offset of 2.7 km/s from the velocity of the H II
Publikováno v:
Publications of the Astronomical Society of Australia. 10:113-117
We have mapped the molecular clouds of Sgr B2 in the 110 → 101 ortho-transition of C3H2 at 18.3 GHz, using the 70-m NASA telescope at Tidbinbilla (beamwidth 55 arcsec). Three clouds show absorption against the Sgr B2 continuum emission at radial ve
Autor:
Ding L; Frontiers Science Center for Transformative Molecules, School of Chemistry and Chemical Engineering, Shanghai Jiao Tong University, Shanghai, 200240, China., Chen Y; Frontiers Science Center for Transformative Molecules, School of Chemistry and Chemical Engineering, Shanghai Jiao Tong University, Shanghai, 200240, China., Sheng Y; Frontiers Science Center for Transformative Molecules, School of Chemistry and Chemical Engineering, Shanghai Jiao Tong University, Shanghai, 200240, China., Yue X; Frontiers Science Center for Transformative Molecules, School of Chemistry and Chemical Engineering, Shanghai Jiao Tong University, Shanghai, 200240, China., Liang Z; Frontiers Science Center for Transformative Molecules, School of Chemistry and Chemical Engineering, Shanghai Jiao Tong University, Shanghai, 200240, China.
Publikováno v:
Angewandte Chemie (International ed. in English) [Angew Chem Int Ed Engl] 2024 Aug 30, pp. e202411933. Date of Electronic Publication: 2024 Aug 30.
Autor:
Wang, Minzhen1 (AUTHOR) wangminzhen@nbu.edu.cn, Zhong, Caiming1 (AUTHOR) zhongcaiming@nbu.edu.cn, Yue, Keyu2 (AUTHOR) 13732849771@163.com, Zheng, Yu2 (AUTHOR) 13694006511@163.com, Jiang, Wenjing3 (AUTHOR) 20211215023@nuist.edu.cn, Wang, Jian3,4,5 (AUTHOR) 003328@nuist.edu.cn
Publikováno v:
Fractal & Fractional. Jun2024, Vol. 8 Issue 6, p320. 22p.