Date and Time of the Query: 2019-08-21 T02:39:25 PDT
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Notes for object NGC 1380

8 note(s) found in NED.

1. 2006MNRAS.371.1912B
Re:NGC 1380
5.1.2 NGC 1380 - Fig. 2 shows that the new data agree extremely well with the
previous observations, but with much improved error bounds. The new data with
their smaller errors and unfolded presentation give some indication of localized
substructure that differs between the two sides of the galaxy. An enhancement in
velocity dispersion within the central ~7 arcsec, first suggested by D'Onofrio
et al. (1995), is strongly confirmed with the new data. It is also notable from
Fig. A2 that this region also shows structure in the h_3_ skewness measure,
indicative of a distinct kinematic component. Interestingly, this feature
coincides with photometric evidence for a distinct component which comprises a
strong variation in isophotal ellipticity and position angle (Caon, Capaccioli &
D'Onofrio 1994).

2. 2005ApJS..157...59L
Re:NGC 1380
NGC 1380 is a lenticular galaxy at a distance of 7.2 Mpc. ULX1 is on the edge of
the galaxy.

3. 2005A&A...440...73C
Re:NGC 1380
NGC 1380: after masking the off-center dust lane, the brightness profile is
smooth and well fitted by a power-law. No flattening is seen before the
resolution limit.

4. 1994CAG1..B...0000S
Re:NGC 1380
FCC 167
Feb 1/2, 1979
103aO + Wr2
45 min
NGC 1380 is a member of the Fornax
Cluster (Ferguson 1989). The spiral pattern of
the massive arms is pronounced and shows
moderately well in this reproduction. The arms
appear to attach to the bulge at position angles of
about 5 o'clock and 11 o'clock in the print here.
The sense of the spiral pattern is clockwise going
from the outside inward.

5. 1985SGC...C...0000C
Re:NGC 1380
Plate 2698
Overexposed center, bright nubs form bar. Many faint galaxies near.

6. 1982ESOU..C...0000L
Re:ESO 033432-3508.4
=ESO 358- G 28
in cluster

7. 1976RC2...C...0000d
Re:NGC 1380
In the Fornax I Cluster
Star 0.85 arcmin south-preceding the nucleus.

8. 1964RC1...C...0000d
Re:NGC 1380
In the Fornax I Cluster.
Very bright nucleus.
Star 0.85 arcmin [south-preceding] the nucleus.
M.N.R.A.S., 111, 526, 1951.

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