NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-05-21 T04:37:16 PDT
Help | Comment | NED Home

Notes for object NGC 1058

10 note(s) found in NED.


1. 2002ApJS..143...73E
Re:NGC 1058
NGC 1058.---Sa: System close to face-on. Centrally peaked nuclear
source. Clear break in surface brightness between the inner and outer
disk. Very faint, flocculent irregular spiral pattern, with tightly
wound arm segments.

2. 2002ApJ...573..306E
Re:NGC 1058
NGC 1058
Radio detection of SN 1961V has been reported by Cowan et al. (1988),
Cowan & Branch (1985), and Cowan et al. (1991). An H{alpha} map from
Cowan et al. (1988) was available for comparison with our sources, but
{alpha} had a position outside (>4' from galaxy center) the H{alpha}
field of view. On the other hand, {beta} was within the field of view
for the H{alpha} map but did not correspond to any H{alpha} emission
region.

3. 2002A&A...392..817F
Re:NGC 1058
3.1 NGC 1058
Two ULX have been detected and both of them appear to have no
evident optical counterpart in the DSS. ULX1 has sufficient counts
to be fitted. The best model is the power law, even though with an
unusual low {GAMMA}=1.1+/-0.3 ({chi^2^=41.1, {nu} = 33). The
0.5-10 keV flux is calculated as 8.5 x 10^-14^ erg cm^-2^ s^-1^,
which corresponds to a luminosity of 1.1 x 10^39^ erg s^-1^. Other
models give worse fits; for example, the black body model with
kT = 0.7 +/- 0.2 keV gives {chi}^2^ = 53.0 for {nu}=33, and we get
an upper limit for the temperature of the inner disk in the MCD
model of kT<4 keV ({chi^2^=43.8, {nu} = 33).

4. 2001ApJS..133...77H
Re:NGC 1058
NGC 1058 (S2). - Not detected. Cowan, Henry, & Branch (1988) obtained
deep radio observations of the site of SN 1961V, but the nucleus of the
galaxy, which lies within 1.3' of the supernova, was not detected at 6 cm
(S_6_ < 0.09 mJy; {DELTA}{theta} = 0.9") or 20 cm (S_20_ < 0.12 mJy;
{DELTA}{theta} = 0.9").

5. 1999A&AS..138..253B
Re:NGC 1058
NGC 1058 - SNe 1961V, 1969L: an elongated patch is clearly visible at
the location of SN 1961V; in V it appears broken up into different
smaller patches: a couple of these are faint and extremely blue in B-V.
The region of SN 1969L is empty. SN 1961V classified as a candidate (see
Table 3).

6. 1994CAG1..B...0000S
Re:NGC 1058
NGC 1023 Group
Sc(s)II-III
PH-1553-B
Oct 8/9, 1956
103aO + GG1
25 min
NGC 1058 is a member of the loose NGC 1023
Group which, in addition to its eponymous
galaxy, contains NGC 891, NGC 925, NGC 1003,
and NGC 1058 shown here.
The redshift, v_o = 221 km/s, for NGC 1058
in Humason, Mayall, and Sandage (1956)
is incorrect. The redshift adopted in the RSA,
based on many later sources, is v_o = 746 km/s,
belying an earlier conclusion, based on the
smaller (incorrect) redshift, that NGC 1058 was
a nearby dwarf spiral.
Individual stars begin to resolve at V = 22.
At a redshift distance of 15 Mpc (i.e., m - M = 30.9),
such stars are of absolute magnitude M_B_ = -9,
which is consistent with the calibration of
brightest resolved blue supergiants in galaxies
with M_B_ = -19 (Sandage and Carlson 1988).

7. 1984AnTok..192.595T
Re:KUG 0240+371
Several knots of HII are in the nucleus and on the arms.

8. 1976RC2...C...0000d
Re:NGC 1058
In the NGC 1023 Group.
Description:
IAU Symp. No.38, 30, 1970.
Photograph:
Ap. J., 139, 514, 1964.
"Stellar Structure", Stars and Stellar Systems, Vol. VIII, p.396, 1965.
P.A.S.P., 82, 894, 1970.
Mem. S.A. Ital., 42, 163, 1971 = Cont. Asiago No. 255.
"Supernovae and SN Remnants", Ap. Space Sc. Lib., Vol. 45, p.215, 1974.
Spectrum:
Old HMS vel.(Vo=221, Source C) rejected.
HII Regions and Distance Modulus:
Ap. J., 194, 559, 1974.
SN1961V
Ap. J., 139, 514, 1964.
"Stellar Structure", Stars and Stellar Systems, VIII, 136, 1965.
Ann. Ap., 27, 319, 1964.
Coll. Int. Novae & SN, CNRS, Paris, 194, 1965.
Info. Bull. Var. Stars, No.196, 1967.
P.A.S.P., 82, 894, 1970.
Ap. J., 167, 89, 1971.
Ap. J., 182, 225, 1973.
"Supernovae and SN Remnants", Ap. Space Sc. Lib., Vol. 45, 143-215, 1974.
SN1969L
IAU Circ. No. 2194, 1969.
IAU Circ. No. 2195, 1969.
IAU Circ. No. 2196, 1969.
Ast. Tsirk. No. 522, 1969
Ast. Tsirk. No. 590, 1970.
Mem. S.A. Ital.42, 163, 1971.
Astr. Ap., 29, 123, 1973.
Ap. J., 185, 303, 1973
Ap. J., 193, 27, 1974.
"Supernovae & SN Remnants", Ap. Space Sc. Lib., Vol. 45, 215, 1974.
Distance Modulus:
Ap. J., 193, 27, 1974.

9. 1973UGC...C...0000N
Re:UGC 02193
SA(rs)c (de Vaucouleurs), Sc- (Holmberg)
SN 1961v, 1969l
Patchy main body, multiple arm pattern
Hints of extremely faint extension to approximately 5. x 5.
`Irregular, thready, bright features' (Morgan)

10. 1964RC1...C...0000d
Re:NGC 1058
In the NGC 1023 Group.
Small, very bright nucleus
in smooth center part.
Many partially resolved arms.
Outer parts are of low surface brightness
Paired with fine anonymous SA(r)0+ at 8 arcmin.
New corrected velocity = +583 km/sec
by Zwicky (Ann. Rep. Mt. Wilson-Palomar, 1962-63):
HII Regions:
Zeit. fur Ap., 50, 168, 1960.
SN 1961
Contr. Osserv. Astr. Asiago, No. 142, 1963.


Back to NED Home