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NGC 7213 ESO288-G043 RA 22:09:16 Dec -47°10.0' Galaxy |
h: "vB,m R, gbM, 45 arcseconds."
Hartung writes: This nebula is a bright
round hazy object about 1.5' across, rising much to the centre with the edges
fading away; it looks like a remote globular cluster . . 7.5cm shows it dimly
but quite definitely.
G. de Vaucouleurs ("Galaxies and the
Universe", Chapter 14 - Nearby Groups of Galaxies) notes that the
Pavo-Indus Cloud includes the NGC 7079 and NGC 7213 Groups. Foreground members
are NGC 7090, IC 5152 & IC 5201. NGC 6970 is a background member. The five
brightest members of the Pavo-Indus Cloud are NGC 7213, NGC 7205, NGC 7049, NGC
7083 & NGC 7144.
Shobbrook (1966, Mon. Not. R. astr. Soc., Vol
131, p351-363) notes that this member of the Grus Cluster has V = 11.41, B-V =
0.90 and U-B = 0.44. It measures 1.55 by 1.55.
Further details appear in: De Vaucouleurs
(1956) Survey of bright galaxies south of -35° declination,
Mem. Mount Stromlo, No. 13. (photographic study, plates taken with the 30-inch
Reynolds reflector, 20-inch diaphragm). In the Notes to the catalogue: see
M.N. 112, 1952, 607. The superior resolving power of the Pretoria 74-inch
photograph shows it to be SAa- with smooth, tightly coiled arms. It is E: in HA
88, 2
15.5-inch f/9 Newtonian:
Lies just southeast of Alpha Grus in the same low-power field. It appears
pretty bright, with two equally bright stars due east, forming a sharp isoceles
with the galaxy at the apex. The galaxy appears round as a globular. (suburban
skies) [AS] |