NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-05-27 T07:01:24 PDT
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Notes for object NGC 3250

6 note(s) found in NED.


1. 2000A&AS..145...71K
Re:NGC 3250
NGC 3250: Counter-rotating disk 9" away from the center of intensity
with a diameter of 3", h_3_ proportional to -v, indicating decoupled
central component kinematics (Bender et al. 1994). The Mg_2_ profile of
this galaxy also features a central depression (Carollo et al. 1993).

2. 1994CAG1..B...0000S
Re:NGC 3250
E3
CD-1408-S/Br
March 23/24, 1980
103aD + GG495
50 min
NGC 3250 is a normal, moderately compact prototypical E3 galaxy.
It is in the rich region of the Hydra-Centaurus Supercluster near
the Antlia Cluster (Sandage 1975b; Ferguson and Sandage 1990), but 4
deg south. A survey and a radial velocity study of the region is given
by Hopp and Materne (1985), where the relation of NGC 3250 to the
neighboring galaxies is set out (their Fig. 1).

3. 1994A&AS..104..179G
Re:NGC 3250
Regular elliptical with low but significant Fourier terms.

4. 1985SGC...C...0000C
Re:NGC 3250
Plate 1363
Faint star superposed. E1 4.2 preceding, SB0 sp 7.2 south-following.

5. 1982ESOU..C...0000L
Re:ESO 102421-3941.3
=ESO 317- G 26
in cluster

6. 1964RC1...C...0000d
Re:NGC 3250
Bright nucleus. There are 2 stars 0.5 arcmin following.


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