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RA: 23h 19m 21.1s
Dec: −42° 15′ 20″
Ch: MSA:1444, U2:415, SA:23
Ref: SIMBAD, Corwin
Type: galaxy, Sc
Mag: B=12.01, V=11.41
Size: 4.365′ x 1.412′
NGC 7599 = IC 5308, which see.
It forms part of the Grus Quartet (NGC 7552, NGC 7582, NGC 7590, NGC 7599)
James Dunlop discovered this object from Paramatta, New South Wales, and included it as No. 477 in his catalogue of 1827. Using a 9-inch f/12 telescope, he described it as "two very small round nebulae, nearly the same RA, and differing about 1' in polar distance." The other object is NGC 7590.
Observed by Sir John Herschel at the Cape of Good Hope with an 18-inch f/13 speculum telescope. He recorded it as "F, pmE, gbM, 3'; the following of two."
Reynolds, J.H. (1921) The spiral nebulae in the zone –40° to –90° (from the Franklin-Adams Plates). MNRAS, 81, 598.
Table p 601: 4x2, pa 90, "BN"
pF, 4'x1', E 55deg, no nucleus; spiural with pBmE central portion and some indications of absorption.
Confirms HOB 22.
Galactic and Extragalactic Studies, III. Photographs of thirty southern nebulae and clusters. Proc. N.A.S., 26, 31-36.
"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).
Shobbrook (1966, Mon. Not. R. astr. Soc., Vol 131, p351-363) notes that this member of the Grus Cluster has V = 11.80, B-V = 0.65 and U-B = -0.01. It measures 3.75 by 1.1. He notes: "It may clearly be seen that NGC 7599 has no significant nucleus. For this object, the brighter central region was offset by about 5 arcseconds to exclude a bright star from the large diaphragm measures."
(Sulentic and Tifft 1973) notes that this is a 12.0 mag galaxy. Their coded description reads S,B,EL,MINC,PCHY * NORTH ARM.
(Astrophysical Journal, 202, 563-582) notes that this galaxy is a member of the IC 1459 Grus Group. Members include NGC 7410, NGC 7412, NGC 7418, NGC 7421, NGC 7424, NGC 7496, NGC 7531, NGC 7552, NGC 7582, NGC 7590, NGC 7599, IC 1459, IC 5267, IC 5269 & IC 5273.
Paturel, G., Petit, C., Kogoshvili, N. et al. (1991) An extragalactic data base. IV. Errors and misprints in catalogues of galaxies. Astrophys.J.Suppl.Ser., 91(3), 371.
NGC 7599 = IC 5308
by Jim Lucyk: Ast.Obj.for South.Tel. (Hartung, 1984).
Hartung notes: "This striking field contains in an area about 16' across three fairly bright spindles differently orientated, all visible with 10.5cm. In order of RA: 4'x1' pa 150 deg; 2' x 0.7' pa 45 deg; 4' x 2' pa 50 deg. The second is the brightest, and the third the faintest and most diffuse."
Steve Coe, observing with a 13" f/5.6, notes: "Faint, pretty large, elongated 2 X 1 in PA 110 at 100X."
Canterbury: pa60. * 1'.4 ESE.
15cm - third in Gru trio. parallel to -90, sev *s inv @ 80x. 140x: 2'.5x1',
reaching 3/4 way to m14.5 * W of SW tip. m13.5 * sup NE side of core.
m12.5 * on E. strong broad concen, no well-def core or nuc, but area SW
of m13.5 * quite distinctly structured w/*ings, knots, dk spots. BS,
30cm - broad, diffuse, little concen @ 140x. occas a vf sm core seen in center.
220x shows elong in pa60, 3'x1'.5. seems to be a few *ings on inner
portions of halo. m12.5 * ESE just out of halo.
Observing site: Fall Star Party
[23h 19m 18s, -42° 16' 0"] Part of a complex smudge with N 7599.
Sky Conditions:The fainter parts of the Milky Way are barely visible.Haziness only visible on the horizon.Atmosphere stable with little interference.
This galaxy has a long extension with an elongated shape which is noticeable at both 57x and 75x.I have found numerous darker areas within the outskirts of this galaxy and that there are plenty of areas of uneven brightness being seen on the far outskirts of this galaxy.The nucleus of this galaxy is slightly condensed and is well defined.The nucleus of this galaxy grows brighter compared to the far outskirts of this galaxy.This galaxy measures 4.7'x 0.7'with PA NE-to-SW.Challenge Rating:Difficult.Chart:No.143,NSOG Vol.3.
The Messier objects
The Bennett objects
The Caldwell list
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