Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Tao, Bojun"'
Autor:
Luo, Yibin, Fan, Lulu, Liang, Yongming, Hu, Weida, Wang, Junxian, Zheng, Zhen-ya, Lin, Zheyu, Tao, Bojun, Lin, Zesen, Cai, Minxuan, Huang, Mengqiu, Wan, Zhen, Tang, Yongling
Hot dust-obscured galaxies (Hot DOGs) are a population of hyperluminous, heavily obscured quasars discovered by the \emph{Wide-field Infrared Survey Explorer} (\emph{WISE}) all-sky survey at high redshift. Observations suggested the growth of these g
Externí odkaz:
http://arxiv.org/abs/2407.16971
Autor:
Chen, Lijun, Zhang, Hong-Xin, Lin, Zesen, Chen, Guangwen, Tao, Bojun, Liang, Zhixiong, Lin, Zheyu, Kong, Xu
The formation mechanism of high-concentration dwarf galaxies is still a mystery. We perform a comparative study of the intrinsic shape of nearby low-mass galaxies with different stellar concentration. The intrinsic shape is parameterized by the inter
Externí odkaz:
http://arxiv.org/abs/2309.05052
Autor:
Tang, Yimeng, Tao, Bojun, Zhang, Hong-Xin, Chen, Guangwen, Gao, Yulong, Lin, Zesen, Yao, Yao, Shi, Yong, Kong, Xu
Publikováno v:
A&A 668, A179 (2022)
NGC 2915 is a unique nearby galaxy that is classified as an isolated blue compact dwarf based on its optical appearance but has an extremely extended H i gas disk with prominent Sd-type spiral arms. To unveil the starburst-triggering mystery of NGC 2
Externí odkaz:
http://arxiv.org/abs/2210.06485
An overdensity of red galaxies around the hyperluminous dust-obscured quasar W1835$+$4355 at $z=2.3$
Autor:
Luo, Yibin, Fan, Lulu, Zou, Hu, Shen, Lu, Lin, Zesen, Hu, Weda, Lin, Zheyu, Tao, Bojun, Chen, Guangwen
\emph{Wide-field Infrared Survey Explorer} all-sky survey has discovered a new population of hot dust-obscured galaxies (Hot DOGs), which has been confirmed to be dusty quasars. Previous statistical studies have found significant overdensities of sub
Externí odkaz:
http://arxiv.org/abs/2207.14312
Akademický článek
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Autor:
Luo, Yibin, Fan, Lulu, Zou, Hu, Shen, Lu, Lin, Zesen, Hu, Weida, Lin, Zheyu, Tao, Bojun, Chen, Guangwen
Publikováno v:
Astrophysical Journal; 8/1/2022, Vol. 935 Issue 2, p1-8, 8p