Date and Time of the Query: 2018-11-13 T13:14:54 PST
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Notes for object NGC 4262

12 note(s) found in NED.

1. 2007AJ....133.2569G
Re:ALFALFA 1-260
1-260.-Resolved disk, elongated southwest (high velocity) to northeast (low
velocity); previous H I cz = 1280 appears to be wrong;

2. 2006MNRAS.369..497K
Re:NGC 4262
This strongly barred object shows inconspicuous metal line gradients. The
H{beta} absorption map shows a mild increase with radius.

3. 2006MNRAS.366.1151S
Re:NGC 4262
Like NGC 3377, this strongly barred galaxy shows an integral-sign pattern in the
gas distribution and a twisted V_gas_field. In addition, this object shows
peculiar asymmetric distributions for the central values of {sigma}_gas_ and for
the [O III]/H{beta} ratio. The gas and stellar kinematics are strongly
decoupled. The unsharp-masked SAURON image shows a bilobated structure
reminiscent of that observed at smaller scales in NGC 2699.

4. 2006ApJS..164..334F
Re:VCC 0355
VCC 355 (NGC 4262).Two dust filaments radiate away from the center in a spiral
pattern, reaching out to a distance of about 4". Other than that, the galaxy
appears regular within this region. Beyond, the isophotes twist (from a position
angle of about -30^deg^ to approximately +20^deg^) and become quite disky.
Inspection of the images reveals the presence of a bar, aligned at a position
angle of +10^deg^ and extending about 27" from side to side. The bar appears
slightly misaligned with respect to the main body of the galaxy at the same
radius. The end of the bar has a "flattened" appearance, resembling a hammer,
although there is no obvious indication of a ring or spiral arms protruding from
it. There is no obvious color feature associated with the bar. There might be a
hint of a compact stellar nucleus from the surface brightness profiles.

5. 2004MNRAS.352..721E
Re:NGC 4262
NGC 4262: This strongly barred galaxy has a remarkably regular velocity
field, the long-axis of the bar being clearly misaligned with the
kinematic minor axis. h_3_ changes sign twice along the major axis.

6. 2004A&A...415..941E
Re:NGC 4262
NGC 4262 (inner disk): Shaw et al. (1995). See Erwin et al. (2004) for
source of bar and disk measurements. The distance is a default value
for the Virgo Cluster, from the HST Key Project study of Freedman
et al. (2001).

7. 1994CAG1..B...0000S
Re:NGC 4262
VCC 355
Hubble Atlas, p. 42
March 24/25, 1955
103aD + GG11
45 min
The high-surface-brightness stubby bar that
emerges from the bulge in NGC 4262 stops short
of the outer edge of the luminosity zone of
intermediate surface brightness, seen here in a
negative print. This form differs from that of NGC
2646, above, where the bar terminates on the
rim of this zone (which is the intermediate disk
seen nearly face on).
A very faint, concentric outer envelope (not
seen in the print here) exists surrounding the two,
zones shown in the main print. These three
luminosity zones are similar to those described
often in the preceding S0 section.

8. 1976RC2...C...0000d
Re:NGC 4262
Ap. J., 146, 28, 1966.
Bull. A.A.S., 5, 349, 1973.

9. 1973UGC...C...0000N
Re:UGC 07365
SB(s)0-? (de Vaucouleurs)

10. 1964RC1...C...0000d
Re:NGC 4262
Extremely bright nucleus in a short bright bar: 0.45 arcmin x 0.1 arcmin.
Smooth bright lens: 0.9 arcmin x 0.8 arcmin. Very faint envelope.
Lund 7 dimensions rejected, nucleus only.
Heidelberg Veroff. Vol. 9, 1926, Lund 9 and HA 88, 4 dimensions are for the
lens only.

11. 1961Hubbl.B...0000S
Re:NGC 4262
Mar. 24/25, 1955
103aD + GG11
45 min
Enlarged 7.1X
The bar has bright ansae which terminate inside the apparent
boundary of the lens. The ansae are not completely
separate from the rest of the bar, as in NGC 2859 (right).
Because of this, the galaxy is a transition case between an
SB02 and SB03 type.

12. 1957HPh....53..275d
Re:NGC 4262
(Plate 13)
Small nucleus in a short, stubby bar (stronger near the
extremities) in a bright diffuse lens.
The nucleus appears larger on this image taken in yellow light.
Compare with NGC 7079 (Plate 9), NGC 3032 (Plate 15)
and NGC 2859 (Plate 16).

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