Date and Time of the Query: 2019-05-18 T23:49:41 PDT
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Notes for object NGC 0289

10 note(s) found in NED.

1. 2005ApJS..160...76B
Re:NGC 0289
The data are noisy and almost 1/3 is excluded as discordant. As a consequence
nothing can be said about the two-dimensional dynamics. These are the first
measures of {sigma}_*_ in NGC 289. See Figure 3.

2. 2003AJ....126..742H
Re:NGC 0289
The morphological classification as determined by us is indicated in
parentheses next to the galaxy name, with our "chaotic circumnuclear
dust" (C) category now not including those galaxies with obvious dust
lanes (DL). Where the classification has already been made by Martini
et al. (2003), we indicate this with "-mp."
3.2. NGC 289 (C)
Figure 1 (top).
Spectra: There is a weak continuum and little extended emission, but
the H{alpha} and [N II] emission lines show characteristics of
Images: As noted by Carollo et al. (2002), a dust lane runs from the
northwest to the southeast, close to the nucleus.

3. 2002ApJS..143...73E
Re:NGC 0289
NGC 289.---SB(r)ab (type example---see Fig. 3d): Strong bar and
aligned elliptical bulge. Symmetric two-arm pattern emerges from the
ends of the bar. Arms are smooth and well-defined. Arms both bifurcate
after ~90deg. Log stretch shows bright ansae at the ends of the bar.

4. 2002AJ....123..159C
Re:NGC 0289
Red (dust) lane across (northwest of red) center

5. 1994CAG1..B...0000S
Re:NGC 0289
Aug 10/11, 1980
103aO + GG385
45 min
The inner spiral pattern of NGC 289 is of
the grand design type. Two arms of high surface
brightness begin near, but not at, the ends of the
bar. As in other cases that are similarly advanced
toward the (r) spiral subtype from the pure NGC 1300
(s) type, each inner arm begins about 15^deg^
downstream from the ends of the bar, winding
outward but missing the opposite arm after half
a revolution. The inner arms in NGC 289 are not
tightly wound. Consequently, there is no
prominent almost-complete inner near-ring, as in
earlier examples of the pattern such as NGC 3081
(SBa; panels 99, 107) and NGC 3185
(SBa; panel 99).
The inner arms cover a high-surface-brightness
disk, outside of which the delicate, thin,
well-formed, very-low-surface-brightness, outer
multiple-arm pattern exists.
These arms are fragments that cannot be
individually traced for more than about a
quarter revolution each.
The brightest knot in one of the inner arms
has an angular diameter (core plus halo) of about
4". It may be a complex of several HII regions,
unresolved at this resolution. The redshift of
NGC 289 is v_o = 1834 km/s.

6. 1985SGC...C...0000C
Re:NGC 0289
Plate 768
Overexposed center (with bar?), (r'): 1.3 x -, faint dist (R'): 5.6 x 4.5
with pretty low surface brightness SB(s)0o superposed 3.2 north-north-preceding.

7. 1982ESOU..C...0000L
Re:ESO 005017-3128.6
=ESO 411- G 25
faint outer arms involved
*small and faint companion 3.4 north preceding

8. 1977A&AS...28....1V
Re:VV 484
Plate 18 Transport out of Large Companions
MCG -05-03-010 = NGC 0289; (12.1m), V_0_=+1907 (RC1).
The companions are apparently not related to the spiral systems, yet
are transported out by means (seemingly) of a massive filament. The
photograph is overexposed and may be misinterpreted.

9. 1976RC2...C...0000d
Re:NGC 0289
Radio Observations:
Austral. J. Phys., 19, 883, 1966.

10. 1964RC1...C...0000d
Re:NGC 0289
Small, bright nucleus.
Bar: 0.55 arcmin x 0.08 arcmin
(r): 0.7 arcmin x 0.4 arcmin
4 main knotty filamentary arms with very faint
outer extensions at a large distance.
Pseudo (R): 2.9 arcmin x 2.5 arcmin.

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