Interpreting the observed 21-cm HI power spectrum

被引:0
|
作者
Minter, A [1 ]
机构
[1] NRAO, Green Bank, WV 24944 USA
来源
SEEING THROUGH THE DUST: THE DETECTION OF HI AND THE EXPLORATION OF THE ISM IN GALAXIES, PROCEEDINGS | 2002年 / 276卷
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper I investigate what factors - both observational and physical - can change the measured slope of the observed 21-cm H-I power spectrum. The following effects can make the observed turbulence appear two dimensional rather than. three dimensional: 1) if the turbulence is contained in a thin filament or slab; 2) if the medium has a high optical depth; and 3) if any method of observation or analysis is used which effectively limits the emission from the medium under study to a thin slab, for example, by analyzing an individual channel map. Straightforward analysis of data can give misleading or incomplete results if these effects axe not taken into account.
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页码:221 / 224
页数:4
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