NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-03-24 T03:51:02 PDT
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Notes for object NGC 4157

4 note(s) found in NED.


1. 2000AJ....119.1592I
Re:NGC 4157
NGC 4157. This galaxy, a member of LGG 258 (Garcia 1993), is a
nondetection in our data. Lower resolution 20 cm images can be found in
Condon 1983, Gioia & Fabbiano 1987, Hummel & van der Hulst 1989, and
Paper I, and they show a somewhat asymmetric distribution with higher
intensities on the southwest major axis. A global equipartition field
strength of 3.26 x 10^-6^ G was derived by Fitt & Alexander (1993). An
HST UV image shows no obvious emission, though a small flux is recorded
by Maoz et al. (1996). Short H I observations, providing global
profiles and position/velocity plots, can be found in Rhee & van Albada
(1996). Our 3{sigma} upper limit corresponds to a radio luminosity of
2 x 10^18^ W Hz^-1^, which is lower than the median radio luminosity of
the supernova remnants in M82. Thus, if supernova remnants exist, they
must have comparatively low luminosities.

2. 1976RC2...C...0000d
Re:NGC 4157
SN1937A
"Supernovae & SN Remnants", Ap. & Space Sc. Lib., Vol. 45, 204, 1974.
SN1955A and Photograph:
P.A.S.P., 77, 456, 1965.

3. 1973UGC...C...0000N
Re:UGC 07183
SAB(s)b? (de Vaucouleurs)
SN 1937a, 1955a
Companion 3.5, 210, 0.3 x 0.1

4. 1964RC1...C...0000d
Re:NGC 4157
Bright center partially obscured by a dark lane on one side. Several knotty,
filamentary arms. Very poorly resolved.
SN 1937
P.A.S.P., 49, 205, 1937.
Ap. J., 88, 291, 1938.
Ap. J., 96, 28, 1942


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