NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-04-21 T17:48:25 PDT
Help | Comment | NED Home

Notes for object NGC 3312

5 note(s) found in NED.


1. 1994CAG1..B...0000S
Re:NGC 3312
Hydra I Cluster
Sab(r)
CD-690-Br
Jan 27/28, 1979
103aO + GG385
45 min
NGC 3312 is the brightest spiral in the region of the Hydra I
Cluster (Abell Cluster 1060). Although its velocity of v_o = 2494 km/s
is smaller than the mean cluster redshift of = 3419 km/s
(Richter, Materne, and Huchtmeier 1982; Richter and Huchtmeier 1983),
these authors accept it as a cluster member; the cluster velocity
dispersion is 681 km/s.
The morphology of NGC 3312 is similar to that of NGC 4826 (Sab;
panel 110) in its large dust complex in the disk. As in NGC 4826, the
dust forms a massive spiral pattern winding through the disk. Knots,
presumably HII regions, are evidence of a modest current
star-formation rate.

2. 1985SGC...C...0000C
Re:NGC 3312
= IC 0629
Plate 530
Overexposed center, very smooth twisted arms.

3. 1982ESOU..C...0000L
Re:ESO 103441-2718.3
=ESO 501- G 43
disturbed
in cluster

4. 1976RC2...C...0000d
Re:NGC 3312
= IC 0629
In the Hydra Cluster?
Colliding pair 22.5 arcmin away.
Peculiar pair 7.5 arcmin away.

5. 1964RC1...C...0000d
Re:NGC 3312
= IC 0629
Extremely bright nucleus. Asymmetric dark lane; perhaps distorted by
NGC 3309-3311.
In the Hydra I Cluster.
Colliding pair(?) at 22.5 arcmin.
Peculiar pair at 7.5 arcmin.


Back to NED Home