Date and Time of the Query: 2019-05-26 T14:13:38 PDT
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Notes for object NGC 3675

9 note(s) found in NED.

1. 2012ApJ...754...67F
Re:NGC 3675
NGC 3675 .SAS3..-The HST F606W image clearly shows a high contrast flocculent
spiral that extends all the way into the center. The velocity dispersion reaches
a maximum of about 110 km s^-1^ at ~=40" and stays rather constant inside of
this radius. The h_3_ moments are anti-correlated with velocity within the bulge
and reach maximum values of about 0.1 at the bulge radius of 8.5".

2. 2002ApJS..143...73E
Re:NGC 3675
NGC 3675.---SB(r)a: Bright nuclear point source embedded in an
elliptical bulge, threaded by a low-contrast bar. Narrow, tightly
wound spiral arms form an inner pseudoring and can be traced for
another full winding outside the ring. Arms are embedded in a clear
interarm disk. The outer arms are very patchy and filamentary.

3. 2001A&A...368...16M
Re:NGC 3675
24. NGC 3675 is an Sb spiral of fairly high inclination. The circular dust
near the centre (very good detectable in a Pa_{alpha}_ snapshot image of
the HST, Boker et al. 1999) leads to some problems with the fit there; this
is visible in the residuum (Fig. 5 in on-line version). Eskridge et al.
(2000) classify NGC 3675 as strongly barred from their analysis of NIR
images in the H filter. We found a bulge component with the same position
angle as the disk and somewhat rounder in projection (Q_b_ = 0.61,
Q_d_ = 0.43), but no signature of a bar.

4. 2000ApJS..129...93F
Re:NGC 3675
NGC 3675. - We detect about 1.5 mJy of low surface brightness
emission on our tapered maps. NVSS detected a 48.9 mJy source, whereas
FIRST measured 8.04 mJy: the source must be strongly resolved. VLA
D-configuration observations at 1.49 GHz (Condon 1987; Gioia & Fabbiano
1987) detected a ~ 50 mJy source, oriented north-south, along the major
axis of the optical galaxy. Condon, Frayer, & Broderick (1991) report a
flux density of 27 mJy at 4.85 GHz and a steep spectral index between
4.8 and 1.4 GHz.

5. 1994CAG1..B...0000S
Re:NGC 3675
April 28/29, 1979
12 min
The high inclination of NGC 3675 permits
the remarkably high dust content to be well seen
in silhouette against the near side of the disk. The
spiral pattern is similar to that of NGC 488,
consisting of a large number of individual spiral
fragments in close concert with fragments of dust
The central bulge in NGC 3675 is smaller
than in NGC 488 or in NGC 2841. These
galaxies are the Sb (MAS) prototype, but all are
earlier in the Sb morphological box than most of
the galaxies on this panel.
The very few knots in the arms of NGC
3675 are presumed to be HII regions. All are
small, not usefully resolving at the 1-2" level.
The redshift of NGC 3675 is v_o = 792 km/s.
The poor resolution into HII regions and stars,
despite the very low redshift, shows that the
current rate of star formation is low.

6. 1976RC2...C...0000d
Re:NGC 3675
Photometry (I.R. 2-20 microns):
Ap. J. (Letters), 159, L165, 1970.
Ap. J. (Letters), 161, L203, 1970.
Ap., J (Letters), 176, L95, 1972.

7. 1973UGC...C...0000N
Re:UGC 06439
SA(s)b (de Vaucouleurs)

8. 1964RC1...C...0000d
Re:NGC 3675
Small, bright, diffuse nucleus. 2 main knotty, regular arms. Strong
absorption lane on one side.
HA 88, 2 dimensions (after Lick 13) are for the bright part only.

9. 1918PLicO..13....9C
Re:NGC 3675
A rather open spiral 3' x 1' in p.a. 0^deg^. Nucleus stellar, and appears
displaced to one side of the central mass because of a well-marked dark lane on
the east. The whorls show a number of very faint, almost stellar condensations.
See Abs. Eff.

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