中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Dust Destruction in Nonradiative Shocks

文献类型:期刊论文

作者Zhu,H.1,2; Slane,P.2; Raymond,J.2; Tian,W. W.1,3,4
刊名The Astrophysical Journal
出版日期2019-09-10
卷号882期号:2
关键词dust, extinction ISM: abundances ISM: supernova remnants
ISSN号0004-637X
DOI10.3847/1538-4357/ab3226
英文摘要Abstract Supernova remnant (SNR) shock waves are the main place where interstellar dust grains are destroyed. However, the dust destruction efficiency in nonradiative shocks is still not well known. One way to estimate the fraction of dust destroyed is to compare the difference between postshock gas abundances and preshock medium total abundances when the preshock elemental depletion factors are known. We compare the postshock gas abundances of 16 SNRs in the Large Magellanic Cloud (LMC) with the LMC interstellar medium abundances that we derived based on 69 slow-rotating early B-type stars. We find that, on average, ~61% of Si-rich dust grains are destroyed in the shock, while the fraction of dust destroyed is only ~40% for Fe-rich dust grains. This result supports the idea that the high depletion of Fe in the diffuse neutral medium is not caused by the resilience of Fe-rich grains but because of faster growth rate. This work also presents a potential way to constrain the chemical composition of interstellar dust.
语种英语
WOS记录号IOP:0004-637X-882-2-AB3226
出版者The American Astronomical Society
源URL[http://ir.bao.ac.cn/handle/114a11/27698]  
专题中国科学院国家天文台
作者单位1.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People's Republic of China zhuhui@bao.ac.cn, tww@bao.ac.cn
2.Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA; pslane@cfa.harvard.edu, jraymond@cfa.harvard.edu
3.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
4.Department of Physics and Astronomy, University of Calgary, Calgary, AB T2N 1N4, Canada
推荐引用方式
GB/T 7714
Zhu,H.,Slane,P.,Raymond,J.,et al. Dust Destruction in Nonradiative Shocks[J]. The Astrophysical Journal,2019,882(2).
APA Zhu,H.,Slane,P.,Raymond,J.,&Tian,W. W..(2019).Dust Destruction in Nonradiative Shocks.The Astrophysical Journal,882(2).
MLA Zhu,H.,et al."Dust Destruction in Nonradiative Shocks".The Astrophysical Journal 882.2(2019).

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来源:国家天文台

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