Mapping the three-dimensional dust extinction towards the supernova remnant S147-the S147 dust cloud

被引:29
作者
Chen, B. -Q. [1 ,2 ]
Liu, X. -W. [1 ,2 ,3 ]
Ren, J. -J. [2 ,4 ]
Yuan, H. -B. [5 ]
Huang, Y. [1 ,2 ]
Yu, B. [5 ]
Xiang, M. -S. [4 ]
Wang, C. [2 ]
Tian, Z. -J. [2 ]
Zhang, H. -W. [2 ]
机构
[1] Yunnan Univ, South Western Inst Astron Res, Kunming 650091, Yunnan, Peoples R China
[2] Peking Univ, Dept Astron, Beijing 100871, Peoples R China
[3] Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
[4] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
[5] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
基金
中国博士后科学基金;
关键词
dust; extinction; ISM: supernova remnants (S147); MHZ MASER EMISSION; GALACTIC ANTICENTRE; MOLECULAR CLOUDS; PSR J0538+2817; MILKY-WAY; GAS; TELESCOPE; COEFFICIENTS; MOTION; RATIO;
D O I
10.1093/mnras/stx2287
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a three-dimensional (3D) extinction analysis in the region towards the supernova remnant (SNR) S147 (G180.0-1.7) using multiband photometric data from the Xuyi Schmidt Telescope Photometric Survey of the Galactic Anticentre (XSTPS-GAC), 2MASS and WISE. We isolate a previously unrecognized dust structure likely to be associated with SNR S147. The structure, which we term as 'S147 dust cloud', is estimated to have a distance d = 1.22 +/- 0.21 kpc, consistent with the conjecture that S147 is associated with pulsar PSR J0538 + 2817. The cloud includes several dense clumps of relatively high extinction that locate on the radio shell of S147 and coincide spatially with the CO and gamma-ray emission features. We conclude that the usage of CO measurements to trace the SNR associated MCs is unavoidably limited by the detection threshold, dust depletion and the difficulty of distance estimates in the outer Galaxy. 3D dust extinction mapping may provide a better way to identify and study SNR-MC interactions.
引用
收藏
页码:3924 / 3935
页数:12
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