Date and Time of the Query: 2019-05-25 T05:20:02 PDT
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Notes for object NGC 1395

9 note(s) found in NED.

1. 2005ApJ...635.1031B
Re:NGC 1395
NGC 1395.-Galactic absorption is present but there is little H_2_ absorption
(about 10^17.5^ cm^-2^), and there is no evidence of Galactic O VI emission,
which would be difficult to detect in this short observation. The strong O VI
line from NGC 1395 would lie at 1037.84 A, a fairly clean part of the spectrum;
there is only an upper limit to this line (Fig. 3).

2. 1994CAG1..B...0000S
Re:NGC 1395
Feb 4/5, 1937
Imp. Ecl.
40 min
NGC 1395 is an isolated, moderately compact, normal E2 galaxy
whose redshift is v_o = 1664 km/s.

3. 1994A&AS..105..341G
Re:NGC 1395
The H{alpha}+[NII] image reveals slightly extended line emission peaked
on the nucleus. Neither our image nor our spectrum confirms the large
extent of the emission-line region reported by Trinchieri & di Serego
Alighieri (1991). The B-I image does not reveal obvious dust absorption.
Since this galaxy has been detected by IRAS at 60 and 100 microns, we
expect the dust to be in a face-on distribution (cf. also the symmetrical
distribution of the ionized gas, Trinchieri & di Serego Alighieri 1991)
Shells revealed in residual image (see also Malin & Carter 1983). Radio
and X-ray source.

4. 1994A&AS..104..179G
Re:NGC 1395
Boxy isophotes. Shells revealed in residual image (see also Malin &
Carter 1983). Detected at 60 and 100 microns by IRAS. Radio and X-ray

5. 1993A&A...280..409B
Re:NGC 1395
NGC 1395: The emission region is almost round in the centre and peaked
at the nucleus. NGC 1395 is a well-studied elliptical which is both an X-
ray source (Canizares et al. 1987) and a shell galaxy (Malin & Carter
1983). H{alpha}+[N II] images have also been obtained by TdiSA and Shields
(1991). Lauer (1985) and Veron-Cetty & Veron (1988) found the stellar
light to be regular with no optical evidence of dust, though our
continuum image suggests there may be a tenuous major-axis dust lane.

6. 1985SGC...C...0000C
Re:NGC 1395
Plate 3620
Overexposed center; very faint broad "jets" to north-preceding and
south-following. Extremely faint much extended corona. 1st in group.

7. 1982ESOU..C...0000L
Re:ESO 033619-2311.4
=ESO 482- G 19
in cluster

8. 1976RC2...C...0000d
Re:NGC 1395
Ap. J., 139, 284, 1964.
Dynamics and Mass Determination:
Ap. J., 139, 284, 1964.

9. 1964RC1...C...0000d
Re:NGC 1395
Very bright center.
Smooth nebulosity.

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