Date and Time of the Query: 2019-05-20 T12:28:22 PDT
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Notes for object NGC 4270

9 note(s) found in NED.

1. 2006MNRAS.369..497K
Re:NGC 4270
The central peaked metal absorption line strengths in this galaxy show evidence
of an increase beyond 10 arcsec along the major axis, giving a small dip around
4-5 arcsec from the centre. The H{beta} absorption map shows no significant

2. 2006MNRAS.366.1151S
Re:NGC 4270
This galaxy shows only fragmented traces of emission and no evidence for
significant absorption features.

3. 2004MNRAS.352..721E
Re:NGC 4270
NGC 4270: At large radii, the velocity field is close to
cylindrical. Inside 10 arcsec the opening angle of the isovelocity
contours decreases, with a corresponding increase in the h_3_
amplitude. The velocity curve in the central ~5 arcsec is flat (Simien &
Prugniel 1997a).

4. 1994CAG1..B...0000S
Re:NGC 4270
VCC 375
March 14/15, 1980
75 min
NGC 4270 is in a complex region of the
Virgo field that contains the W cloud, which is
more distant than the Virgo Cluster proper. The
large, very-low-surface-brightness dwarf VCC
367, on the main print near the lower right-hand
border, is classed ImV? in the VCC with no
decision as to cluster membership.
NGC 4270 itself has the characteristic S0
zone morphology (seen best in the insert) of
bulge, inner lens, and outer extended envelope.

5. 1994A&AS..105..481M
Re:NGC 4270
NGC 4270: An S0 with a disky lens surrounded by a boxy and rather
peculiar envelope.

6. 1976RC2...C...0000d
Re:NGC 4270
= Holm 368c
In group with NGC 4273.
Ap. J., 146, 28, 1966.

7. 1973UGC...C...0000N
Re:UGC 07376
S0 (de Vaucouleurs), S0 (Holmberg)

8. 1964RC1...C...0000d
Re:NGC 4270
= Holm 368c
In a group with NGC 4268 and NGC 4273.

9. 1918PLicO..13....9C
Re:NGC 4270
An oval with bright center, 1' x 0.3', in p.a. 105^deg^, probably a spiral. This
is near the center of a remarkable field which contains thirteen N. G. C.
objects, and eighty-one other small and faint nebulae. 81 s.n.

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