INTERSTELLAR-MEDIUM MAPPING IN M82 THROUGH LIGHT ECHOES AROUND SUPERNOVA 2014J
文献类型：期刊论文
| 作者 | Yang, Yi1; Wang, Lifan1,2,3 ; Baade, Dietrich; Brown, Peter. J.1; Cracraft, Misty4; Hoflich, Peter A.5; Maund, Justyn6; Patat, Ferdinando3; Sparks, William B.4; Spyromilio, Jason3
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| 刊名 | ASTROPHYSICAL JOURNAL
 |
| 出版日期 | 2017 |
| 卷号 | 834期号:1页码:15 |
| ISSN号 | 0004-637X |
| 关键词 | circumstellar matter dust, extinction galaxies: individual (M82) ISM: structure polarization supernovae: individual (SN 2014J) |
| DOI | 10.3847/1538-4357/834/1/60 |
| 通讯作者 | Yang, Yi(ngc4594@physics.tamu.edu) |
| 英文摘要 | We present multiple-epoch measurements of the size and surface brightness of the light echoes from supernova (SN) 2014J in the nearby starburst galaxy M82. Hubble Space Telescope (HST) ACS/WFC images were taken similar to 277 and similar to 416 days after B-band maximum in the filters F475W, F606W, and F775W. Observations with HST WFC3/UVIS images at epochs similar to 216 and similar to 365 days are included for a more complete analysis. The images reveal the temporal evolution of at least two major light-echo components. The first one exhibits a filled ring structure with position-angle-dependent intensity. This radially extended, diffuse echo indicates the presence of an inhomogeneous interstellar dust cloud ranging from similar to 100 to similar to 500 pc in the foreground of the SN. The second echo component appears as an unresolved luminous quarter-circle arc centered on the SN. The wavelength dependence of scattering measured in different dust components suggests that the dust producing the luminous arc favors smaller grain sizes, while that causing the diffuse light echo may have sizes similar to those of the Milky Way dust. Smaller grains can produce an optical depth consistent with that along the supernova-Earth line of sight measured by previous studies around maximum light. Therefore, it is possible that the dust slab from which the luminous arc arises is also responsible for most of the extinction toward SN. 2014J. The optical depths determined from the Milky Way-like dust in the scattering matters are lower than the optical depth produced by the dust slab. |
| WOS关键词 | LARGE-MAGELLANIC-CLOUD ; CORE-COLLAPSE SUPERNOVAE ; HIGH-RESOLUTION SPECTRA ; IA SUPERNOVA ; SN 2014J ; SPACE-TELESCOPE ; CIRCUMSTELLAR DUST ; GREAT ERUPTION ; ETA-CARINAE ; MILKY-WAY |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| 出版者 | IOP PUBLISHING LTD |
| WOS记录号 | WOS:000391745300005 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/23342]  |
| 专题 | 中国科学院紫金山天文台 |
| 通讯作者 | Yang, Yi |
| 作者单位 | 1.Texas A&M Univ, Dept Phys & Astron, George P & Cynthia Woods Mitchell Inst Fundamenta, 4242 TAMU, College Stn, TX 77843 USA 2.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China 3.European Org Astron Res Southern Hemisphere ESO, Karl Schwarzschild Str 2, D-85748 Garching, Germany 4.Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA 5.Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA 6.Univ Sheffield, Dept Phys & Astron, Hicks Bldg,Hounsfield Rd, Sheffield S3 7RH, S Yorkshire, England 7.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China 8.Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China 9.Univ Texas Austin, Dept Astron, RLM 15308, Austin, TX 78712 USA 10.Univ Texas Austin, McDonald Observ, Austin, TX 78712 USA |
| 推荐引用方式 GB/T 7714 | Yang, Yi,Wang, Lifan,Baade, Dietrich,et al. INTERSTELLAR-MEDIUM MAPPING IN M82 THROUGH LIGHT ECHOES AROUND SUPERNOVA 2014J[J]. ASTROPHYSICAL JOURNAL,2017,834(1):15. |
| APA | Yang, Yi.,Wang, Lifan.,Baade, Dietrich.,Brown, Peter. J..,Cracraft, Misty.,...&Wheeler, J. Craig.(2017).INTERSTELLAR-MEDIUM MAPPING IN M82 THROUGH LIGHT ECHOES AROUND SUPERNOVA 2014J.ASTROPHYSICAL JOURNAL,834(1),15. |
| MLA | Yang, Yi,et al."INTERSTELLAR-MEDIUM MAPPING IN M82 THROUGH LIGHT ECHOES AROUND SUPERNOVA 2014J".ASTROPHYSICAL JOURNAL 834.1(2017):15. |
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来源：紫金山天文台
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