Zobrazeno 1 - 10
of 169
pro vyhledávání: '"Jin Long Xu"'
Autor:
Yingjie, Li, Ye, Xu, Jin-Long, Xu, Dejian, Liu, Jingjing, Li, Zehao, Lin, Peng, Jiang, Shuaibo, Bian, Chaojie, Hao, Xiuhui, Chen
We observed the high-mass star-forming region G176.51+00.20 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST) with the 19-beam tracking observational mode. This is a pilot work of searching for neutral stellar winds traced by ato
Externí odkaz:
http://arxiv.org/abs/2207.06602
Autor:
Yingjie, Li, Ye, Xu, Jin-Long, Xu, Dejian, Liu, Jingjing, Li, Zehao, Lin, Peng, Jiang, Shuaibo, Bian, Chaojie, Hao, Xiuhui, Chen
Publikováno v:
ASTROPHYS. J. LETT. 933 (2022) L26
Using the Five-hundred-meter Aperture Spherical radio Telescope (FAST) 19-beam tracking observational mode, high sensitivity and high-velocity resolution HI spectral lines have been observed toward the high-mass star-forming region G176.51+00.20. Thi
Externí odkaz:
http://arxiv.org/abs/2207.06601
Autor:
Chuan-Peng Zhang, Ming Zhu, Peng Jiang, Cheng Cheng, Jin-Long Xu, Nai-Ping Yu, Xiao-Lan Liu, Bo Zhang
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 276, Iss 1, p 6 (2024)
The FAST All Sky H I survey (FASHI) will cover the entire observable sky (∼22,000 square degrees) with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). With the currently released data, we perform an untargeted survey of 21 cm H i
Externí odkaz:
https://doaj.org/article/37734815a8f74a0ab3be005e74238247
Publikováno v:
The Astrophysical Journal, Vol 971, Iss 2, p 131 (2024)
The FAST All Sky H i survey (FASHI) is broader in frequency band and sky volume, and deeper in detection sensitivity than the Arecibo Legacy Fast ALFA survey. To efficiently expand the sample of OH megamasers (OHMs), whose strongest line has a rest f
Externí odkaz:
https://doaj.org/article/0d52fd4c9eec4d379a1645976b2d476d
Autor:
Jin-Long Xu, Ming Zhu, Kelley M. Hess, Naiping Yu, Chuan-Peng Zhang, Xiao-Lan Liu, Mei Ai, Peng Jiang, Jie Wang
Publikováno v:
The Astrophysical Journal Letters, Vol 958, Iss 2, p L31 (2023)
Based on the atomic-hydrogen (H i ) observations using the Five-hundred-meter Aperture Spherical radio Telescope, we present a detailed study of the gas-rich massive S0 galaxy NGC 1023 in a nearby galaxy group. The presence of a H i extended warped d
Externí odkaz:
https://doaj.org/article/4b62f5a0a48d483b8f256d4f051f63ff
Publikováno v:
The Astrophysical Journal Letters, Vol 944, Iss 2, p L40 (2023)
Based on a new H i survey using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), combined with the Pan-STARRS1 images, we identified an isolated H i cloud without any optical counterpart, named FAST J0139+4328. The newly discovered H
Externí odkaz:
https://doaj.org/article/6022fe3eb8bc470288c5c51d32456c5e
Publikováno v:
Polymer Testing, Vol 111, Iss , Pp 107595- (2022)
Developing durable and sustainable flame retardant (FR) polyamide 6 (PA6) fabric is of great interest. Herein, an eco-friendly Maillard reaction product (MRP) was developed by carbonyl-amino condensation between glucose and thiourea. Then, the functi
Externí odkaz:
https://doaj.org/article/27cbe55cb20241b08a54093eb60c2dce
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:737-742
With the aim to study the extended H i environment around dwarf galaxies in the local universe, we performed a high-sensitivity H i observation of the DDO 168 and DDO 167 pair using the Five-hundred-meter Aperture Spherical Radio Telescope (FAST). We
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 521:2719-2728
We observed the classical interacting galaxy M51 with FAST and obtain high sensitivity HI image with column density down to 3.8 $\times$ 10$^{18}$ cm$^{-2}$. In the image we can see a diffuse extended envelope around the system and several new tidal
Publikováno v:
CyTA - Journal of Food, Vol 15, Iss 1, Pp 105-109 (2017)
Two casein plasteins were prepared from the Neutrase-catalyzed plastein reaction of casein hydrolysates in the presence of proline and phenylalanine, respectively, and assessed for their antihypertensive activities at 300 mg/kg body using rat model.
Externí odkaz:
https://doaj.org/article/109b16455f174cabac8a1a2b9cb5a728