NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-05-27 T00:29:04 PDT
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Notes for object NGC 5857

8 note(s) found in NED.


1. 2001A&A...379...54H
Re:KPG 455A
KPG455A. The galaxy is classified as SB(s)b and our (B-I) and
sharp/filtered images show a bright nuclear region and two faint wrapped
spiral arms resembling an inner ring. It is difficult to trace the presence
of a bar, although the bulge region is elongated. The spiral pattern
becomes diffuse at the outer parts. We classify this galaxy as SA(r)b.
The (B-V)_T_^0^ colour is representative of S0a-Sa types.

2. 1999A&AS..138..253B
Re:NGC 5857
NGC 5857 - SN 1950H, 1955M: a compact and blue patch is found at the
location of SN 1950H. This SN lies close to the nuclear part of the
galaxy.

3. 1998A&AS..130..333T
Re:PGC 053995
NGC5857
Pair with NGC5859 also in the beam. Both have similar type, magnitude
and velocity. The HI profile is consequently confused.

4. 1976RC2...C...0000d
Re:NGC 5857
= Kara[72] 455a.
Pair with NGC 5859 at 2.0 arcmin.
SN1950H and SN1955M
P.A.S.P., 86, 516, 1974 (with photograph).

5. 1973UGC...C...0000N
Re:UGC 09724
SB(s)b (de Vaucouleurs)
Paired with UGC 09728 at 2.0, 120

6. 1964RC1...C...0000d
Re:NGC 5857
Very small, very bright nucleus in a bright lens: 0.3 arcmin x 0.25 arcmin.
Pseudo (r): 0.3 arcmin x 0.2 arcmin. 2 main, regular arms.
Heidelberg Veroff. Vol. 9, 1926 dimensions are for the lens only.
B magnitude (Source C) is for NGC 5857 + NGC 5859.
Interacting (?) pair with NGC 5859 at 2.0 arcmin.

7. 1956AJ.....61...97H
Re:NGC 5857
HMS Note No. 185
Slit on elongated nuclear region, which corresponds closely
with the major axis. Lines may be inclined, but inclination
is uncertain because of weak plate.

8. 1918PLicO..13....9C
Re:NGC 5857
NGC 5857 and NGC 5859
Vol. VIII, Plate 50. Described as a double nebulae in the N. G. C. 5857 is a
bright, compact, somewhat oval spiral 1' long, with a bright, almost stellar
nucleus; whorls of uniform texture. 5859 is 2.6' x 0.6' in p.a. 130^deg^ ;
apparently a {phi}-type spiral seen at a considerable angle, with most of the
matter in one large whorl. The nucleus is almost stellar; there are a few
condensations. Moderately bright. 5 s.n.


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