Date and Time of the Query: 2019-05-23 T22:17:52 PDT
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Notes for object NGC 4707

5 note(s) found in NED.

1. 2002A&A...387..821G
Re:UGC 07971
UGC 7971 (NGC 4707)
The H{alpha} emission of this magellanic spiral is concentrated in
a few bright HII regions at the periphery of the main body. It is thus
impossible to draw a velocity field and we just give the approximate
velocity values for the 5 brighter HII regions, from which one can
hardly guess the position of the major axis. The derived rotation
curve is not very significant because of the paucity of the H{alpha}
emission. The WHISP HI data show a large HI hole in the center of the
galaxy, the HI gas appearing as a ring surrounding the main optical
body. The WHISP HI velocity field suggests a solid body rotation with
a small amplitude, as confirmed by the HI rotation curve derived by
Swaters (1999). No clear comparison with our H{alpha} curve is possible
because of the high dispersion of our points. Indeed, the low values
of the rotation velocities we find in the outer parts, on the receding
side, are produced by two HII regions only, the motions of which may
not be representative at all of the average motion in the disk.

2. 1976RC2...C...0000d
Re:NGC 4707
= DDO 150
= I Zw 043
Many emission knots; small nucleus or star.

3. 1973UGC...C...0000N
Re:UGC 07971
I Zw 43, DDO 150
"Very blue irregular... with many blue knots (possible neutral stellar nucleus,
or star superposed, m_p_ = 15.0)" (CGPG)
S IV-V or S V (DDO)

4. 1971CGPG..C...0000Z
Re:CGPG 1246.1+5127
I Zw 043
NGC 4707
Very blue irregular .
With many blue knots (possibly neutral stellar nucleus, or star superposed,
m(pg) = 15.0)
m(pg)= 15.2 [CGCG]

5. 1966AJ.....71..922v
Re:DDO 150
= NGC 4707.
Star projected on nucleus.

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