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Date and Time of the Query: 2019-04-25 T11:55:58 PDT
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Notes for object NGC 6137

7 note(s) found in NED.


1. 2005MNRAS.364.1253V
Re:NGC 6137
NGC 6137. We estimate that ~20 per cent of the 850-{mu}m flux from this
elliptical galaxy could be due to synchrotron contamination from a radio source
associated with the galaxy (Vlahakis et al. in preparation). Although only the
submm emission to the W of the galaxy coincides with a noisy bolometer we note
that this observation had a tilted sky.

2. 2005ApJ...618..635G
Re:NGC 6137
1621+38 (NGC 6137) (Fig. 17)
This head-tail radio galaxy has bright, short, symmetric jets
oriented north-south on the kiloparsec scale and an extended
low-brightness tail to the east (Fanti et al. 1987). In our VLBI
image a bright core and a one-sided jet are present. The parsec-scale
jet is slightly misaligned but oriented on the same side with respect
to the core as the brighter kiloparsec-scale jet (~160^deg^ VLBI,
90^deg^ VLA).

3. 2002AJ....124..675C
Re:UGC 10364
The NVSS identification of this head-tail radio source
(Parma et al. 1986) is correct despite the large optical/NVSS offset.

4. 1999MNRAS.310...30C
Re:B2 1621+38
B2 1621+38 was analysed by Feretti et al. (1995), who found a
point-source contribution of <= 50 per cent of the total X-ray flux.
Our analysis is consistent with this result; we find the point-source
contribution to be 18 +/- 4 per cent.

5. 1986A&AS...64..135P
Re:B2 1621+38
The diffuse tail has a direction perpendicular to a smaller scale jet
emanating from the nucleus. See also Ekers et al (1978) for a discussion
of the environment. A high resolution map is given by O'Dea and Owen (1985).

6. 1976RC2...C...0000d
Re:NGC 6137
= B2 1621+38
In Abell 2199.

7. 1973UGC...C...0000N
Re:UGC 10364
Paired with 16 21.2 +38 04 at 1.7, 338, 0.7 x 0.6, S0, m=15.5
Companion 3.9, 340, 0.30 x 0.15
Several galaxies in vicinity


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