Date and Time of the Query: 2019-06-20 T02:48:24 PDT
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Notes for object NGC 5068

12 note(s) found in NED.

1. 2002A&A...391...83B
Re:NGC 5068
NGC 5068 (Fig. 13) has strong radio emission from the small bar and
star-forming regions. Weak polarization has been detected at {lambda}6 cm
in the southern part.

2. 1999A&AS..136...35S
Re:NGC 5068
NGC 5068 -- From five giant HII regions surveyed by D'Odorico et al.
(1983) in this galaxy, two exhibit a broad emission feature at the blue
WR bump.

3. 1997A&A...326..449M
Re:NGC 5068
NGC 5068. The H II regions in the stellar bar are unevenly distributed along
the major axis but are also present in the entire stellar bar. The dust
distribution in the bar is quite complex, with lanes crossing the bar
perpendicularly. The stellar bar is much larger than the H{alpha} bar. The
global O/H gradient the galaxy appears relatively shallow (-0.046 dex kpc^-1^;
Ryder 1995).

4. 1994CAG1..B...0000S
Re:NGC 5068
April 4/5, 1981
75 min
The angular size of NGC 5068 is large at
D_25_ = 6.9'. It is highly resolved into HII-region
candidates and individual brightest stars that
could be as bright as B = 18.5 but which must be
individually separated from the HII-region
candidates before the data can be interpreted.
Star formation is occurring in the bar. Many
classical OB associations can be identified in the
arms. The largest HII region resolves at a
diameter (halo) of about 4". The redshift of
NGC 5068 is v_o = 443 km/s.

5. 1993ApJS...88..415R
Re:NGC 5068
Here is yet another example of how lopsided the H II region distribution
in late-type spirals can be, even those exhibiting well-organized spiral
structure. A number of giant H II region complexes to the west are
visible even in blue light photographs (e.g., SB88), but only two such
objects are found in the eastern arms. Several much fainter and diffuse
H II regions do help fill out the star-forming disk and trace the spiral
pattern. After continuum subtraction, the bar is still quite prominent in
H{alpha} due to a thin chain of H II regions running across the small
bulge. McCall, Rybski, & Shields (1985) have measured oxygen abundances
in four H II regions in NGC 5068.
This is one of two galaxies in this atlas (the other being NGC 2835)
also included in the photographic atlas of Hodge & Kennicutt (1983). A
comparison with their microfiche reproductions illustrates the
substantial gain in contrast and sensitivity recently made possible with
improved imaging systems.

6. 1985SGC...C...0000C
Re:NGC 5068
Plate 2394
Overexposed bar, many knots; similar to M33. Superposed on group.

7. 1982ESOU..C...0000L
Re:ESO 131613-2046.6
=ESO 576- G 29
in cluster

8. 1976RC2...C...0000d
Re:NGC 5068
HII Regions:
"Atlas and Catalogue", Univ. Washington, Seattle, 1966.
Ap. J., 155, 417, 1969.
Ap. J., 194, 559, 1974.
Distance Modulus:
Ap. J., 194, 559, 1974.
Radio Observations:
Australian J. Phys., 19, 883, 1966.

9. 1974UGCA..C...0000N
Re:UGCA 345
UGCA 345:
= NGC 5068
SAB(rs)cd (RC1)

10. 1968MCG4..C...0000V
Re:MCG -03-34-046
A large number of small HII regions. {omega}=0 degrees, {mu}1=70
degrees, {mu}2=74 degrees, {phi}1=360 degrees, {phi}2=330 degrees,
l1=1.4, l2=1.8. Type: Sand - SBc, vB - S(B)c III-IV, Morg - aB-al and
afSI (B), Vauc - SAB(rs)cd. Redshift: +408. Photo: AJ 61 No. 3.
Flattened companion 18 mag i=III, I=3 at 3.9 arcmin north.

11. 1964RC1...C...0000d
Re:NGC 5068
Short, bright bar: 0.8 arcmin x 0.1 arcmin with a very small nucleus.
Pseudo (r): 1.6 arcmin x 1.9 arcmin. 2 main, knotty, partially resolved arms
with many branches.
Helwan 30 and 38 minor axis dimensions are much too small.
A.J., 61, 97, 1956.

12. 1956AJ.....61...97H
Re:NGC 5068
HMS Note No. 166
Slit on short central bar. broad absorption lines on strong
night sky spectrum (HMS Plate IVt).

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