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Date and Time of the Query: 2019-04-25 T06:45:10 PDT
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Notes for object NGC 2434

7 note(s) found in NED.


1. 2001MNRAS.322..702M
Re:NGC 2434
NGC 2434 As mentioned in Section 2, Rix et al. (1997) have used
Scharzschild's method to construct spherical models of this galaxy. Their
models required a dark halo with v_c_ ~ 300 km s^-1^ at around r_eff_.
Our results are in very good agreement. We re-iterate, however, that if
this galaxy were flattened along the line of sight these spherical models
would underestimate the true circular velocity.

2. 2000A&AS..144...53K
Re:NGC 2434
The SB-profile is composite of V-band HST-data from Carollo et al.
(1997) out to 10 arcsec and B-band ground-based data by Carollo &
Danziger (1994). The HST data were shifted by 0.88 mag to give a smooth
transition between the two data sets. Note that Faber et al. (1989) give
an effective radius of 81 arcsec whereas Rix et al. (1997) took 24
arcsec. In our analysis we used the latter value, but this is used only
as a scaling constant and has no influence on any of the derived
quantities.

3. 1994CAG1..B...0000S
Re:NGC 2434
E0
CD-739-S
Feb 3/4, 1979
103aD + GG495
45 min
NGC 2434 is a normal prototype E0 with no bright dwarf companions.

4. 1994A&AS..105..433L
Re:NGC 2434
NGC 2434 (Fig. 13). At both position angles we find very little rotation.
The velocity dispersion profiles are very noisy, but look rather normal
for an E0 galaxy.

5. 1994A&AS..105..433L
Re:NGC 2434
NGC 2434 (Fig. 13). At both position angles we find very little rotation.
The velocity dispersion profiles are very noisy, but look rather normal
for an E0 galaxy.

6. 1985SGC...C...0000C
Re:NGC 2434
Plate 1164r
Overexposed center, star 1.1 north-preceding.
Plate 2009r
Overexposed center, pretty bright star superposed on
envelope 1.1 north-preceding. NGC 2442 16.7 south-following.

7. 1982ESOU..C...0000L
Re:ESO 073459-6910.3
=ESO 059- G 05
in ESO 059- G 08 group


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