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首页> 外文期刊>The Astrophysical journal >ZEEMAN EFFECT OBSERVATIONS OF H I EMISSION PROFILES. I. MAGNETIC FIELD LIMITS FOR THREE REGIONS BASED ON OBSERVATIONS CORRECTED FOR POLARIZED BEAM STRUCTURE
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ZEEMAN EFFECT OBSERVATIONS OF H I EMISSION PROFILES. I. MAGNETIC FIELD LIMITS FOR THREE REGIONS BASED ON OBSERVATIONS CORRECTED FOR POLARIZED BEAM STRUCTURE

机译:H I排放特征的塞曼效应观察。一,基于偏光梁结构校正观测的三个区域的磁场极限

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摘要

Magnetic field mapping of three H I features, toward MBM 12, MBM 40, and H0928 + 02, was attempted using 21 cm Zeeman effect observations corrected for sidelobe signals. A detailed description of errors introduced into the observations through interaction between H I brightness structure around the source direction and polarized beam structure is given. After corrections were applied to the data, no unambiguous magnetic field effects were found. The previous claim by this author of a field toward NPS 20, associated with MBM 40, is not confirmed. For each mapped area the individual field fits were averaged, and the results indicate 0.25 ± 0.12 μG for the MBM 40 region (error 1 σ), 0.48 ± 0.31 μG for H0928 + 02, and -0.29 ± 0.38 μG for those directions toward MBM 12 where the data were judged to be reliable. The implied upper limits of 0.36 μG for the MBM 40 region and less than 1.0 μG for the other two suggest that the magnetic field strength in diffuse H I observed with a 22′ beam is far lower than has heretofore been recognized.
机译:尝试使用针对旁瓣信号校正的21厘米塞曼效应观测结果,对MBI 12,MBM 40和H0928 + 02的三个H I特征进行磁场映射。给出了通过围绕光源方向的H I亮度结构与偏振光束结构之间的相互作用而引入到观测结果中的误差的详细描述。在对数据进行校正之后,没有发现明确的磁场效应。该作者先前对与MBM 40相关联的NPS 20领域的主张没有得到证实。对于每个映射区域,均对各个场拟合进行平均,结果表明MBM 40区域为0.25±0.12μG(误差1σ),H0928 + 02为0.48±0.31μG,MBM方向为-0.29±0.38μG 12个数据被认为是可靠的地方。 MBM 40区域的隐含上限为0.36μG,其他两个区域的隐含上限小于1.0μG,这表明用22'光束观察到的散射H I中的磁场强度远低于迄今公认的强度。

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