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Date and Time of the Query: 2019-05-25 T02:50:39 PDT
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Notes for object NGC 3245

19 note(s) found in NED.


1. 2012ApJ...754...67F
Re:NGC 3245
NGC 3245 .LAR0*.-The HST F547M image reveals a nuclear dust disk while the
larger scale bulge morphology is classical. This galaxy potentially hosts a lens
(de Vaucouleurs et al. 1991). The rotational velocity exhibits a shelf reaching
from about 3" out to the bulge radius at 15". The velocity dispersion profile
rises steadily toward the center. The h_3_ moments are anti-correlated with
velocity inward of 5". At 5" they reach a maximum and then drop to zero toward
the bulge radius. The h_4_ are compatible with zero at the bulge radius (r_b_ =
8.5 arcsec) but with decreasing radius briefly drop to about -0.05 at +/-5".
Finally inside of 2" they become compatible with zero.

2. 2008MNRAS.386.2242H
Re:NGC 3245
NGC 3115 and NGC 3245 have boxy bulges, while their bulge Sersic index
is n~= 4 . We suggest central classical bulges and outer boxy bulges
coexist in these galaxies.

3. 2008MNRAS.386.2242H
Re:NGC 3245
NGC 3115 and NGC 3245 have boxy bulges, while their bulge Sersic index is
n~=4. We suggest central classical bulges and outer boxy bulges coexist in these
galaxies.

4. 2006A&A...460...45G
Re:NGC 3245
NGC 3245 (UGC 5663). No unresolved nuclear source was detected in the (4.5-8.0*
keV) band image. This contrasts with the analysis by Filho et al. (2004) who,
when making use of the same Chandra data, conclude that there is a hard nuclear
X-ray source coincident with the optical nucleus. The luminosity they calculate
with a fixed {GAMMA} = 1.7 is less than a factor of 2 fainter than ours.

5. 2006A&A...453...27C
Re:UGC 05663
UGC 5663: Filho et al. (2004) find a hard nuclear X-ray source,spatially
coincident with the optical nucleus. The spectrum of the nuclear source is
fitted with a power-law ({GAMMA} fixed at value 1.7).

6. 2005A&A...440...73C
Re:UGC 05663
UGC 5663: despite the presence of extended patches of dust, the masking
procedure allows us to derive its brightness profile which is well fitted by a
Nuker law.

7. 2004A&A...418..429F
Re:NGC 3245
NGC 3245 There is a hard nuclear X-ray source coincident with the
optical nucleus. The soft X-ray emission is resolved and extended (~6")
in the North-South direction.

8. 2002ApJS..142..223F
Re:NGC 3245
NGC 3245. NVSS reports a 7.2 mJy source, similar to the 6 mJy detected
within FIRST. Wrobel & Heeschen (1991) find an unresolved 3.3 mJy core
at 5 GHz, 5" resolution. Judging from these data, the source could be
flat spectrum and compact.

9. 2002ApJ...574..740T
Re:NGC 3245
NGC 3245.
The velocity dispersion is obtained from Simien & Prugniel (1998).

10. 1997ApJS..112..391H
Re:NGC 3245
NGC 3245.--Along with NGC 5005, the line profiles of this galaxy exhibit one of
the most complicated velocity structures in this survey (Fig. 10b). The
rotation curve rises very steeply within the central 4" in the two-dimensional
spectrum, causing each line to have a double-horned profile. Despite this
complexity, each line can be well modeled by a combination of three Gaussian
components: one for the nucleus and one each for the receding and approaching
sides of the disk. While the same combination of components fits [N II] and
[S II], the central (nuclear) component of H{alpha} is weaker than the two disk
components, as is obvious from the dip in the center of the profile. This is
simply a manifestation of the higher [N II]/H and [S II]/H ratios for the LINER
component centered on the nucleus (classified in Paper III as a transition
object). A very faint (f_blend_~12%), broad (FWHM~2650 km s^-1^) component of
H{alpha} is suggested by our decomposition, but the result, unfortunately, is
ambiguous, because it seems to depend on the choice of template model used in
the starlight subtraction.

11. 1995ApJS...98..477H
Re:NGC 3245
All the emission lines of NGC 3245 are double peaked, resulting from its
unusually steep rotation curve. The line profiles are reminiscent of
those of NGC 488 and NGC 7479.

12. 1994CAG1..B...0000S
Re:NGC 3245
Hubble Atlas, p. 4
S0_1_(5)
(P)
H-2160-H
Jan 29/30, 1941
Cramer Hi Speed Sp
60 min
NGC 3245 has a pronounced prototypical
S0_1_ three-zone structure where the separations
between the zones appear to be sharp. The
central E0-like bulge is burned out in this print.
The lower-surface-brightness (but still quite
high) inner disk (called the lens in the Hubble
Atlas) is seen in the facing print as the E5-like
flattened structure. The faint outer envelope,
equally flattened, is very well shown in this print.
The print here has been made from the same
Mount Wilson 100-inch plate that was used for
the illustration in the Hubble Atlas. The outer
envelope is better seen on the negative print here
than on the positive print there. The central,
more circular bulge is shown in the insert print
of the same galaxy on the next panel.

13. 1994CAG1..B...0000S
Re:NGC 3245
Hubble Atlas, p. 4
S0_1_(5)
(P)
PH-8017-S
Feb 3/4, 1981
103aO
12 min
NGC 3245 is also shown on the preceding
panel from a different original negative. The
description there applies to the image here as
well. The insert was made from the Mount Wilson
100-inch plate H-2160-H.

14. 1994A&AS..105..481M
Re:NGC 3245
NGC 3245: This S0 shows an important disk, with inner-ring and outer-
lens, mixed in an envelope of the thD class (see Fig. 4). There is also a
curious gray asymmetry along the minor-axis.

15. 1976RC2...C...0000d
Re:NGC 3245
Non-interacting pair with NGC 3245A at 8.8 arcmin.
Photometry: (5 Color)
A.J., 73, 313, 1968.

16. 1973UGC...C...0000N
Re:UGC 05663
SA(r)0/a:? (de Vaucouleurs)
See UGC 05662

17. 1964RC1...C...0000d
Re:NGC 3245
Extremely bright nucleus in a very bright, smooth lens: 0.6 arcmin x
0.3 arcmin. Diffuse envelope.
Non-interacting pair with NGC 3245A at 8.8 arcmin.

18. 1961Hubbl.B...0000S
Re:NGC 3245
S01
H-2160-H
Jan. 29/30, 1941
Cr-Hi-Sp-Sp
60 min
Enlarged 9.0X
NGC 3245 is one of the best examples of S01 shown on the
page. The outer envelope is quite extensive. It is often
difficult to classify a galaxy which is near the E or S01
boundary. NGC 3245 is a "late" S01, and there is no
difficulty of classification.
The original plate of NGC 3245 shows that the nucleus is
spherical and the lens and outer envelope are elliptical.

19. 1918PLicO..13....9C
Re:NGC 3245
An oval 2' long; nucleus very bright, and outer portions quite faint. Indis-
tinct traces of spiral character. 1 s.n.


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