Diffuse radio source.
Jan 31/Feb 1, 1976
103aO + GG13
Three arms emerge from the central region
of NGC 3756. As the arms wind outward they fill
the area of the disk, being of the massive variety
in the sense of Reynolds (1927a,b) lacking a
thin, well-defined form.
The redshift of NGC 3756 is v_o = 1372 km/s.
The galaxy is in the region of the Ursa Major
Cluster but is considered to be a probable
Splendid S galaxy with knotty arms.
Non-interacting pair with NGC 3738 at 16 arcmin
Observatory, 88, 239, 1968.
SAB(rs)bc (de Vaucouleurs), Sc- (Holmberg)
See UGC 06554, UGC 06565
Small, bright nucleus. Pseudo (r?): 0.55 arcmin x 0.25 arcmin. 2 main knotty
filamentary arms with many branches. Non-interacting pair with NGC 3738 at
See also HA 105, 230, 1937.
Ap. J., 85, 325, 1937.