Erratum: Dust yields in clumpy supernova shells: SN 1987A revisited
Erratum: Dust yields in clumpy supernova shells: SN 1987A revisited
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勘误：块状超新星壳中的尘埃产量：SN 1987A 重新审视
DOI：
10.1111/j.1365-2966.2007.11994.x
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发表时间：
2007
影响因子：
4.8
通讯作者：
Ercolano B
中科院分区：
文献类型：
--
作者：
Ercolano B
这篇论文《超新星壳层中的尘埃产量：SN 1987 A修订版》发表于2009年11月。没有R. 375，753-763，（2007）。我们已经确定了一个错误的版本中的MOCASSIN代码用于辐射传输模型的尘埃超新星信封。误差影响了尘埃发射率计算的概率密度函数。结果是图2-11、13和14所示的红外光谱形状是不正确的。该错误影响了2.02版本。14比2.02 41的代码（版本2.02。21被用于这项工作）-没有其他出版的作品受到影响。在优化过程中引入的误差有效地消除了发射系数的频率依赖性，将红外光谱能量分布（SED）减少为多个温度的黑体的组合，并通过颗粒的自吸收进行修改。只有用于蒙特卡罗确定红外尘埃发射的概率密度函数（PDF）受到误差的影响，SED的光学部分不受影响，因为后者由PDF控制以吸收灰尘，这是正确的。我们文章中提出的所有主要结论是
The paper ‘Dust yields in clumpy supernova shells: SN 1987A revisited’, was published in Mon. Not. R. Astron. Soc. 375, 753–763,(2007). We have identified an error in the version of the MOCASSIN code used for the radiative transfer modelling of the dusty supernova envelope. The error affected the probability density functions for the calculation of dust emissivities. The result is that the infrared spectral shapes shown in figs 2–11, 13 and 14 are not correct. The error affected versions 2.02. 14 to 2.02. 41 of the code (version 2.02. 21 was used for this work)–no other published work is affected. The error, introduced during an optimization exercise, effectively removed the frequency dependence from the emission coefficient, reducing the infrared spectral energy distribution (SED) to a combination of blackbodies of multiple temperatures, modified by selfabsorption by the grains.Only the probability density functions (PDFs) used for the Monte Carlo determination of the infrared dust emission were affected by the error, with the optical part of the SED not being affected, as the latter is controlled by the PDFs for dust absorption, which were correct. All the main conclusions presented in our article are
DOI：
10.1111/j.1365-2966.2006.11336.x
发表时间：
2006-11
影响因子：
4.8
作者：
B. Ercolano;M. Barlow;B. Sugerman
通讯作者：
B. Ercolano;M. Barlow;B. Sugerman