Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Shuaibo Bian"'
Autor:
Dejian Liu, Ye Xu, YingJie Li, Zehao Lin, Chaojie Hao, WenJin Yang, Jingjing Li, Xinrong Liu, Yiwei Dong, Shuaibo Bian, Deyun Kong
Publikováno v:
The Astrophysical Journal, Vol 964, Iss 1, p 93 (2024)
We identify a molecular bubble, and study the star formation and its feedback in the S Mon region, using multiple molecular lines, young stellar objects (YSOs), and infrared data. We revisit the distance to S Mon, ∼722 ± 9 pc, using Gaia Data Rele
Externí odkaz:
https://doaj.org/article/ff9841643fe248c5af8dda963b65553a
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 268, Iss 2, p 46 (2023)
Using young open clusters and O–B2-type stars in Gaia Data Release 3, we investigate the kinematics of the local spiral structure. In general, the young sources in the outer spiral arms may present larger peculiar motions than those in the inner sp
Externí odkaz:
https://doaj.org/article/64fe42809d5a427285572fe8bdd98de1
Autor:
Yiwei Dong, Yan Sun, Ye Xu, Zehao Lin, Shuaibo Bian, Chaojie Hao, Dejian Liu, Yingjie Li, Ji Yang, Yang Su, Xin Zhou, Shaobo Zhang, Qing-Zeng Yan, Zhiwei Chen
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 268, Iss 1, p 1 (2023)
We present the results of an unbiased ^12 CO/ ^13 CO/C ^18 O ( J = 1–0) survey in a portion of the third Galactic quadrant (TGQ): 219.°75 ≤ l ≤ 229.°75 and −5.°25 ≤ b ≤ 5.°25. The high-resolution and high-sensitivity data sets help to
Externí odkaz:
https://doaj.org/article/a14858e4b77b4f74831712da445da770
Publikováno v:
The Astrophysical Journal, Vol 952, Iss 1, p 64 (2023)
Since the hypervelocity stars were discovered in the Milky Way, various mechanisms have been proposed to explain these runaway stars. Up to now, however, the dominant ejected mechanism of hypervelocity stars is still unclear. As the largest and close
Externí odkaz:
https://doaj.org/article/031527dfb7e64196a824aecf05ad23a8
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
Establishing the period--Wesenheit relation requires independent and accurate distance measurements of classical Cepheids (DCEPs). The precise distance provided by an associated open cluster independently calibrates the period--Wesenheit relation of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f23079800acc9321e94d70f031fe2d9
http://arxiv.org/abs/2210.02086
http://arxiv.org/abs/2210.02086
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a335533dee1bc8957111a36e1837cd09
http://arxiv.org/abs/2207.06602
http://arxiv.org/abs/2207.06602
Using the cross-matched data of Gaia EDR3 and the 2MASS Point Source Catalog, a sample of RC stars with parallax accuracies better than 20% is identified and used to reveal the nearby spiral pattern traced by old stars. As shown in the overdensity di
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::03113ea09817e19f47298c7990d5aaa0
Autor:
Yingjie Li, Ye Xu, Jin-Long Xu, Dejian Liu, Jingjing Li, Zehao Lin, Peng Jiang, Shuaibo Bian, Chaojie Hao, Xiuhui Chen
Publikováno v:
The Astrophysical Journal Letters. 933: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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::19fbb3c9e300f072575e9ebe5c088a5e
https://doi.org/10.3847/2041-8213/ac7b7c
https://doi.org/10.3847/2041-8213/ac7b7c