The distance measurements of supernova remnants in the fourth Galactic quadrant

被引：0

作者：

Su-Su Shan ^{[1
,2
]}

Hui Zhu ^{[1
,3
]}

Wen-Wu Tian ^{[1
,2
]}

Hai-Yan Zhang ^{[1
]}

Ai-Yuan Yang ^{[4
]}

Meng-Fei Zhang ^{[1
,2
]}

机构：

[1] Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences

[2] School of Astronomy, University of Chinese Academy of Sciences

[3] Harvard-Smithsonian Center for Astrophysics

[4] Max-Planck-Institut für Radioastronomie

来源：

ResearchinAstronomyandAstrophysics | 2019年 / 19卷 / 07期

基金：

中国国家自然科学基金;

关键词：

ISM:supernova remnants; ISM:dust; extinction; stars:distances;

D O I：

暂无

中图分类号：

P145.3 [新星和超新星];

学科分类号：

070401 ;

摘要：

We take advantage of red clump stars to build the relation of the optical extinction(AV) and distance in each direction of supernova remnants(SNRs) with known extinction in the fourth Galactic quadrant. The distances of nine SNRs are determined well by this method. Their uncertainties range from 10% to30%, which are significantly improved for eight SNRs, G279.0+1.1, G284.3–1.8, G296.1–0.5, G299.2–2.9,G308.4–1.4, G309.2–0.6, G309.8–2.6 and G332.4–0.4. In addition, SNR G284.3–1.8 with the new distance of 5.5 kpc is not likely associated with the PSR J1016–5857 at 3 kpc.

引用

页码：27 / 34

页数：8

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