A cold nearby cloud inside the Local Bubble

被引：41

作者：

Meyer, David M.

Lauroesch, J. T.

Heiles, Carl

Peek, J. E. G.

Engelhorn, Kyle

机构：

[1] Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA

[2] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

来源：

ASTROPHYSICAL JOURNAL | 2006年 / 650卷 / 01期

基金：

美国国家科学基金会;

关键词：

ISM : atoms; ISM : clouds; ISM : structure; solar neighborhood;

D O I：

10.1086/508658

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The high-latitude Galactic H I cloud toward the extragalactic radio source 3C 225 is characterized by very narrow 21 cm emission and absorption indicative of a very low H I spin temperature of about 20 K. Through high-resolution optical spectroscopy, we report the detection of strong, very narrow Na I absorption corresponding to this cloud toward a number of nearby stars. Assuming that the turbulent H I and Na I motions are similar, we derive a cloud temperature of 20(-8)(+6) K (in complete agreement with the 21 cm results) and a line-of-sight turbulent velocity of km s(-1) from a comparison of the H I and Na I absorption line widths. We also place a 0.37 +/- 0.08 firm upper limit of 45 pc on the distance of the cloud, which situates it well inside the Local Bubble in this direction and makes it the nearest known cold diffuse cloud discovered to date.

引用

页码：L67 / L70

页数：4

共 18 条

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