NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2018-11-16 T07:40:36 PST
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Notes for object NGC 0428

10 note(s) found in NED.


1. 2002ApJS..143...73E
Re:NGC 0428
NGC 428.---SBm (type example---see Fig. 3k): Nuclear point source
embedded in an asymmetric inner disk. No true bulge. Outer disk has
numerous star-forming knots, and evidence for two very asymmetric
spiral arms. The NW arm is fairly tightly wrapped, and the better
defined of the two in its inner part. It has several very bright knots
through ~60deg of winding to the east. It then becomes very diffuse
and poorly defined but can still be traced as a low surface brightness
(LSB) feature through a winding angle of ~180deg. The SE arm is very
loosely wrapped and has LSB. It can be followed for ~100deg to the
west.

2. 2002AJ....124..675C
Re:UGC 00763
NVSS and FSC sources offset to bright, knotty arm.

3. 1996AJ....111..712H
Re:NGC 0428
0110+006 (NGC 428). This galaxy is large and irregular, with a very knotty
appearance throughout. Two bar-like bright regions suggest that an interaction
may be occurring, and one of the bars has more bright knots than the other. The
galaxy is not detected at radio wavelengths by NH.
The reddest knots lie at the edges of the bars or in the outer parts of the
whole system. The bluest objects lie mostly in the bright bar but also are
concentrated in the second bar and in the outer arm. No knots have the colour
and magnitude of main sequence stars and dereddening places them all above the
100 M_sun_ line for single stars.

4. 1994CAG1..B...0000S
Re:NGC 0428
Sc(s)III
PH-7562-S
Nov 7/8, 1978
103aO
12 min
The semi-chaotic pattern seen here is similar
to that in NGC 5645 on the preceding panel. The
surface brightness of the inner disk is high. Many
HII regions exist in the bright part of one of the
major arms on one side of the image. Useful
resolution into individual stars from the ground
seems difficult.
The redshift of NGC 428 is v_o = 1311 km/s.

5. 1993A&AS...97..887B
Re:NGC 0428
NGC 428
No CO was detected in the center and in both lines down to a level of
0.6 K km/s, assuming the HI velocity range.

6. 1976RC2...C...0000d
Re:NGC 0428
HII Regions and Distance Modulus:
Ap. J. 194, 559, 1974.

7. 1973UGC...C...0000N
Re:UGC 00763
SAB(s)m (de Vaucouleurs), Sc+ (Holmberg)
Patchy central region, almost dissolved spiral structure, patchy loop south
and south-following center

8. 1964RC1...C...0000d
Re:NGC 0428
Bright, partly resolved weak bar.
Weak, partly resolved filamentary arms, one stronger.
Emission-line object.
Low surface brightness.
Lick (1956) velocity is for 2 emission patches.

9. 1956AJ.....61...97H
Re:NGC 0428
HMS Note No. 011
Only {lambda} 3727 in two emission patches:
42 arcsec [north-west] of the center, on the major axis.
48 arcsec [south-east] of the center, on the major axis.

10. 1918PLicO..13....9C
Re:NGC 0428
This is an extremely irregular mass of nebulosity 4' x 2.2' It shows an
irregular looped structure with numerous stellar condensations; probably a
greatly distorted spiral. 47 s.n.


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