Issue |
A&A
Volume 436, Number 3, June IV 2005
|
|
---|---|---|
Page(s) | L53 - L56 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:200500122 | |
Published online | 03 June 2005 |
Letter to the Editor
Tiny H I clouds in the local ISM
1
ASTRON, Postbox 2, 7990 AA Dwingeloo, The Netherlands e-mail: braun@astron.nl
2
National Radio Astronomy Observatory, Socorro, NM 87801, USA e-mail: nkanekar@aoc.nrao.edu
Received:
22
April
2005
Accepted:
9
May
2005
We report deep, high spectral resolution WSRT 21 cm
observations of four high latitude compact radio sources, that have revealed a
new population of tiny, discrete clouds in the diffuse ISM, with peak optical
depths
%,
column densities of
0.4–
cm-2 and core temperatures of 20–80 K. Imaging
detections confirm these low column densities and imply linear core
dimensions of a few thousand AU, assuming a distance of 100 pc. The physical
origin of these tiny
structures and their distribution in the ISM
is at present unknown. Further observations will be required to determine
whether they are a ubiquitous component of the ISM.
Key words: ISM: clouds / ISM: bubbles / stars: winds, outflows / Galaxy: solar neighbourhood
© ESO, 2005
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