Date and Time of the Query: 2019-05-24 T01:29:31 PDT
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Notes for object NGC 4464

6 note(s) found in NED.

1. 2007MNRAS.377..759S
Re:NGC 4464
NGC 4464: this galaxy, situated in the Virgo cluster, shows a power-law inner
profile (Faber et al. 1997; Lauer et al. 2005).

2. 2006ApJS..164..334F
Re:VCC 1178
VCC 1178 (NGC 4464).A compact nucleus is clearly visible in the color image, but
barely discernible in the surface brightness profiles. The isophotes appear

3. 2001MNRAS.326..473H
Re:NGC 4464
A9 NGC 4464
NGC 4464 is a member of the Virgo cluster and has an uncertain
classification as a spiral galaxy in RC3. Observed by L95, a_4_ was
measured to be almost zero for the central 4 arcsec, and ellipticity
{epsilon} ~ 0.35 for 1 arcsec <~ r <~ 10 arcsec.
For radii |r| <~ 10 arcsec along the major axis, significant
asymmetrical and symmetrical deviations of the LOSVD from a Gaussian are
indicated by non-zero h_3_ and h_4_ (see Fig. A9). The measurements of
h_4_ are of large amplitude and change sign with increasing radius. The
large amplitude of h_3_ for the major axis suggests the presence of
multiple components of different kinematics along the line of sight.
For |r| <~ 5 arcsec, the measurements are consistent with the superposition
of a bulge and an additional, more rotationally supported, component. At
greater radii, the rotation begins to decrease, suggesting that the more
rotationally supported (perhaps disc) component has a scalelength of
~5 arcsec, and that at |r| > 5 arcsec a more slowly rotating bulge
component begins to dominate the galaxy light. We note that the kinematic
measurements for these galaxies are similar to those of NGC 5582.

4. 1976RC2...C...0000d
Re:NGC 4464
Ap. J., 179, 731, 1973.

5. 1973UGC...C...0000N
Re:UGC 07619
E2 (de Vaucouleurs)

6. 1918PLicO..13....9C
Re:NGC 4464
Quite bright; slightly oval, 0.3' long; no spiral structure discernible.

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