Date and Time of the Query: 2019-03-26 T08:01:23 PDT
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Notes for object NGC 6926

6 note(s) found in NED.

1. 2002ApJS..143...47D
Re:IRAS 20305-0211
IRAS 20305-0211 (NGC 6926).---This galaxy is paired with NGC 6929 with
a separation of 4' (de Vaucouleurs, de Vaucouleurs, & Corwin 1976).
This is a barred spiral galaxy with particularly strong emission in the
northern spiral arm. This strong emission is also seen in our H{alpha}
image, with this spiral arm being the brightest H{alpha} emitting
region of the galaxy. Additional weaker star-forming regions can be
observed along the rest of the spiral arms, but H{alpha} emission is
lacking in the nucleus. (Corbett et al. 2002b) classifies this galaxy
as a starburst.

2. 2002AJ....124..675C
Re:UGC 11588
The large galaxy UGC 11588 is the correct identification of
F20304-0211 despite the large optical/FSC offset.

3. 1998A&AS..130..333T
Re:PGC 064939
NGC6926, VV 621
Sbc, pair with NGC6929 (S0) which could disturb the signal. However, the
atypical shape of the profile could rather be due to intrinsic pattern:
"very bright patchy arc tends to disrupt the spiral pattern" (from

4. 1985ApJS...57..643D
Re:VV 621
Distorted spiral.
Small elliptical located 4 arcmin east (not connected).
See Barbieri, C., Casini, C., Heidmann, J., Di Serego, S.,
and Zambon, M. 1979, Astr. Ap. Suppl., 37, 559.

5. 1976RC2...C...0000d
Re:NGC 6926
Pair with NGC 6929 at 4.0 arcmin

6. 1973UGC...C...0000N
Re:UGC 11588
Bright very patchy arcs, tendency to disrupted spiral pattern
Paired with 20 30.8 -02 12 = NGC 6929 at 4.0, 98, 0.7 x 0.6, m=14.9

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