High Resolution Observations of the Magnetic Field in IC 342

High Resolution Observations of the Magnetic Field in IC 342
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IC 342 中磁场的高分辨率观测

DOI:
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发表时间:
1993
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影响因子:
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通讯作者:
M. Krause
M. Krause
中科院分区:
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文献类型:
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作者:
M. Krause

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众所周知,正面螺旋星系IC342具有轴对称螺旋磁场(ASS),其磁力线至少在所分析的5KPC1到13KPC1的径向范围内到处向内定向(Krause等人,1989a;Sokoloff等人,1992)。相对于银河系平面,ASS场的配置似乎是均匀的。
The face-on spiral galaxy IC 342 is known to possess an axisymmetric spiral magnetic field (ASS) with magnetic field lines being orientated inwards everywhere at least in the analyzed radial range between 5 and 13 kpc1 (Krause et al., 1989a; Sokoloff et al., 1992). The ASS field configuration seems to be even with respect to the galactic plane.