A&A 370, L26-L30 (2001)
DOI: 10.1051/0004-6361:20010333
Deep H I observations of the compact high-velocity cloud HVC 125+41-207
C. Brüns1, 2, J. Kerp1 and A. Pagels11 Radioastronomisches Institut der Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
2 The Australia Telescope National Facility, CSIRO, PO Box 76, Epping NSW 1710, Australia
(Received 14 December 2000 / Accepted 7 March 2001 )
Abstract
We present deep HI observations of the compact high-velocity
cloud HVC 125+41-207 using the 100-m Effelsberg telescope.
Our goal was in particular to study the warm neutral medium (WNM) in detail.
The Effelsberg data reveals a two phase core/halo structure -one component
with a velocity width of
km s-1 (Westerbork data
show
km s-1, Braun & Burton 2000) and
one with
km s-1.
The column density distribution of the warmer component is highly asymmetric
and shows a head-tail structure. We performed a Gaussian decomposition of
the cloud and found that 52% of the HI mass of the cloud is in the WNM.
24% of the WNM is located in the tail.
The overall structure and the systematic
variation of the observational parameters radial velocity, velocity
dispersion and column density indicate that this cloud is currently
interacting with the ambient medium.
The Westerbork HI data of this HVC (Braun & Burton
2000) reveals an interesting dense condensation. Assuming that this
condensation is virialized and in pressure equilibrium with the ambient medium, we derive
a distance of 130 kpc for HVC 125+41-207.
Following these considerations, it is possible to constrain the
parameters
cm-3 and
K of the intergalactic medium of the
Local Group.
Key words: ISM: clouds, kinematics and dynamics -- Galaxy: halo -- galaxies: intergalactic medium
Offprint request: C. Brüns, cbruens@astro.uni-bonn.de
SIMBAD Objects
© ESO 2001

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