Issue |
A&A
Volume 374, Number 2, August I 2001
|
|
---|---|---|
Page(s) | 682 - 690 | |
Section | The Sun | |
DOI | https://doi.org/10.1051/0004-6361:20010737 | |
Published online | 15 August 2001 |
The HI supershell GS061+00+51 and its neighbours
1
Astronomical Institute, Academy of Sciences of the Czech Republic, BočníII 1401, 141 31 Prague 4, Czech Republic
2
MPIfR, Auf dem Hügel 69, 53121 Bonn, Germany
Corresponding author: S. Ehlerová, sona@alnitak.ig.cas.cz
Received:
27
February
2001
Accepted:
18
May
2001
We describe Hi observations of a field
in the Milky Way centered on
,
made by the
Effelsberg radiotelescope. The field contains one previously identified
Hi supershell, GS061+00+51 (Heiles [CITE]); apart from it we find several
new structures. We also study the Hi distribution in the vicinity of
four Hii regions, S86, S87, S88 and S89.
We confirm the existence of the shell GS061+00+51, and we find
that it has two smaller neighbours, spherical shells with
. We identify at least one more
regular shell at
; and
one blown-out shell at
. In two cases we are
able to connect Hii regions with features in the Hi distribution
(S86 and S87), in two other cases no connection is found. Apart from
quite regular Hi shells we see a number of non-coherent objects,
which are probably a result of the turbulence in the interstellar
medium.
Key words: ISM: bubbles / ISM: supernova remnants / ISM: Hii regions / radio lines: ISM
© ESO, 2001
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