A high galactic latitude HI 21 cm-line absorption survey using the GMRT: I. Observations and spectra

被引:15
作者
Mohan, R [1 ]
Dwarakanath, KS [1 ]
Srinivasan, G [1 ]
机构
[1] Raman Res Inst, Bangalore 560080, Karnataka, India
关键词
ISM : clouds; kinematics and dynamics; radio lines : ISM;
D O I
10.1007/BF02702370
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have used the Giant Meterwave Radio Telescope (GMRT) to measure the Galactic HI 21-cm line absorption towards 102 extragalactic radio continuum sources, located at high (\b\ > 15degrees) Galactic latitudes. The Declination coverage of the present survey is delta greater than or similar to - 45degrees. With a mean rms optical depth of similar to 0.003, this is the most sensitive Galactic HI 21-cm line absorption survey to date. To supplement the absorption data, we have extracted the HI 21-cm line emission profiles towards these 102 lines of sight from the Leiden Dwingeloo Survey of Galactic neutral hydrogen. We have carried out a Gaussian fitting analysis to identify the discrete absorption and emission components in these profiles. In this paper, we present the spectra and the components. A subsequent paper will discuss the interpretation of these results.
引用
收藏
页码:143 / 183
页数:41
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