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Date and Time of the Query: 2018-12-13 T10:48:00 PST
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Notes for object NGC 0863

9 note(s) found in NED.


1. 2004ApJ...613..682P
Re:MRK 0590
Mrk 590. The H{beta} profile in the rms spectrum in the first data set
(JD 2,448,090-2,448,323) seems anomalously narrow, although the rms
spectrum for this data set is significantly noisier than for the other
rms spectra (note the lower value of F_var_ in Table 5). We have
therefore excluded the first data set from the mass analysis, since the
line width is questionable although the lag measurement seems
trustworthy.

2. 2003ApJS..148..327S
Re:Mrk 0590
5.5. Mrk 590
This Seyfert 1 galaxy has a slightly extended NLR (Fig. 5, bottom
left), with dimensions of 1.1" x 1.5" (560 x 770 pc), and major axis
along P.A. = -5^deg^. This emission does not resemble a conically
shaped NLR. Most of the extended [O III] emission comes from the
region north of the nucleus and is misaligned by ~50^deg^ relative to
the host galaxy major axis. The radio emission (Schmitt et al. 2001b)
is unresolved.

3. 2002AJ....124..675C
Re:UGC 01727
Seyfert 1.2.

4. 1998ApJ...501...82P
Re:MRK 0590
Markarian 590 was included in our program because our early IDS observations
showed that it underwent enormous H{beta} variations. Additional observations
indicated that the emission-line variations were concentrated in the core of the
line; the wings apparently vary much less, leading Ferland, Korista, & Peterson
(1990) to suggest that the high radial velocity H{beta} emission arises in an
optically thin gas. A preliminary version of a subset of our CCD observations
(JD 2448090-2448323) has been previously published (Peterson et al. 1993).

5. 1998AJ....116.2682C
Re:IRAS 02120-0059
NGC 863, Mrk 590. Seyfert 1.2. Optical position from Clements (1981).
The compact radio core has a flux density S = 5.0 mJy at 2.29 GHz on the
275 km Parkes-Tidbinbilla Interferometer (PTI) baseline (Roy et al.
1994). VLA A-configuration 8.4 GHz map of the core in Kukula et al.
(1995), C-configuration 8.4 GHz flux density 4.38 mJy. The original IRAS
PSC position is quite far from NGC 863, but the FSC2 position
{alpha} = 02^h^12^m^00.3^s^, {delta} = -01^deg^00'04" is in good
agreement with the accurate optical and radio positions.

6. 1995MNRAS.276.1262K
Re:MRK 0590
Markarian 590: (NGC 863, UGC 03374) Type 1. Host galaxy: Sa (UGC). Radio:
as with 0152+06, the C-array object is slightly resolved even though the
majority of the flux comes from the unresolved source in the A-array map.

7. 1986AnTok..212.127T
Re:KUG 0212-009
Face-on S or S0 galaxy with the extended halo.

8. 1976RC2...C...0000d
Re:NGC 0863
= MRK 0590
Seyfert galaxy.
Spectrum:
Astrofizika, 10, 485, 1974.

9. 1973UGC...C...0000N
Re:UGC 01727
See UGC 01713


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