NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-06-26 T15:38:26 PDT
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Notes for object CGCG 097-125

1 note(s) found in NED.


1. 2002A&A...384..383I
Re:CGCG 097-125
The field around galaxies CGCG 97-114, CGCG 97-120 and CGCG 97-125 deserves
special attention. Each one of them shows H{alpha} emission. However
CGCG 97-120 is not listed in Table 4 because its radial velocity,
5595 km s^-1^, (de Vaucouleurs 1991) is out of the transmitance window of
the on-band filter. Instead, CGCG 97-114 and CGCG 97-125 have very similar
velocities lying in our filter range: 8293 km s^-1^ (de Vaucouleurs 1991)
and 8271 km s^-1^ (Haynes et al. 1997) respectively. If these galaxies
form a sub-group within Abell 1367 ( = 6500 km s^-1^), this entity
must have a very high velocity dispersion. The group coincides in position
with the X-ray cluster center (Donnelly et al. 1998). CGCG 97-120 is a
very H I deficient galaxy (def(H I) = 0.9, Chincarini et al. 1983),
indicating that it has passed through the cluster center, while
CGCG 97-125 is not (def(H I) = -0.21, Haynes et al. 1997). No H I
measurement is available for CGCG 97-114, because it lies close (in space
and in velocity) to CGCG 97-125.


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