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Date and Time of the Query: 2019-05-19 T02:57:06 PDT
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Notes for object IC 3370

9 note(s) found in NED.


1. 2005A&A...440...73C
Re:IC 3370
IC 3370: dust patches cover a large fraction of the nuclear regions of this
galaxy. The resulting profile is quite complex and no fit has been performed.

2. 2000A&AS..141..385V
Re:IC 3370
C-41 = IC 3370.
(G,N) Though generally considered a box-shaped elliptical, with a
prominent dust lane in its inner regions, there is evidence for
cylindrical rotation and X-shaped isophotes (Jarvis 1987; Goudfrooij
1994a, 1994b; Keel & Wu 1995; Penereiro et al. 1994). Two possible
nuclei in addition to the primary one were identified by Forbes et al.
(1994). The central stellar velocity dispersion is 202 km s^-1^ (see
Prugniel & Simien 1996), and the maximum stellar rotation velocity about
95 km s^-1^ (Carollo et al. 1993; Jarvis 1987). Detected at Green Bank,
but not at Nancay (with a higher rms noise). No other object was found
within the Nancay search area.

3. 1994CAG1..B...0000S
Re:IC 3370
E2 pec
CD-1286-S/Br
March 9/10, 1980
103aD + GG495
45 min
There is structure interior to the otherwise nearly normal
exterior E2 image of IC 3370 here. On a short-exposure du Pont plate,
a bright nucleus of finite size (3 arcsec) is surrounded by a faint
disk buried within the first 10% of the image shown here.

4. 1994AJ....107...99R
Re:IC 3370
C-41 = IC 3370. Although generally considered a box-shaped elliptical,
there is evidence for cylindrical rotation and X-shaped isophotes (Jarvis
1987, Whitmore & Bell 1988, Seitzer and Schweizer 1990). NED lists one
other galaxy within the GB 140' beam and three more just outside it, one
of which has a redshift nearly identical to that of IC 3370. Our
extremely marginal detection of 5.1 x 10^8^ M_sun_ of H I is shifted by
300 km s^-1^ from the optically-determined redshift of the galaxy. We
find M_HI_/L_B_ < 0.01, which makes this system the most gas-poor galaxy
in our sample.

5. 1994A&AS..105..341G
Re:IC 3370
Prominent dustlane in central region (see also Sadler & Gerhard 1985),
associated with H{alpha}+[NII] emission. Nearly square isophotes at
larger radii (cf. Jarvis 1987). Molecular gas has been detected in this
galaxy (Lees et al. 1991). Detected by IRAS at 60 and 100 microns.
Nuclear radio source.

6. 1994A&AS..104..179G
Re:IC 3370
Isophotes are significantly distorted in the inner ~ 8" due to a
prominent dustlane, especially in B and V. This galaxy has nearly square
isophotes at larger radii (cf. Jarvis 1987), modeled by the ellipse
fitting program as a large PA twist and significant S4 amplitudes.
Detected by IRAS at 60 & 100 microns. Nuclear radio source.

7. 1985SGC...C...0000C
Re:IC 3370
Plate 1477r
Overexposed rectangular nucleus with plumes at corners. Possible I0.

8. 1982ESOU..C...0000L
Re:ESO 122457-3903.7
=ESO 322- G 14
in cluster

9. 1964RC1...C...0000d
Re:IC 3370
Bright nucleus: 0.5 arcmin x 0.4 arcmin.


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