U 456
18:36 to 19:48
-61° to -72°
Pav
May-Nov

FEATURED OBJECTS: NGC 6744, NGC 6684.

NGC 6744
ESO104-G042
RA 19:09:45
Dec -63°51.3'
Galaxy

Dunlop 262: he observed it on 3 occasions and described it as “a pretty large very faint nebula, about 5' or 6' diameter, slightly bright towards the centre; a minute star is north of the nebula, and two stars of the 7th mag preceding.”

h: “pretty bright, round, after first very gradually, then suddenly very much brighter in the middle; total diam. 2', but that of the bright part 15 arcseconds.” The second observation was recorded as “bright, round, gradually pretty much brighter in the middle, 60 arcseconds, resolvable.”

Hartung, observing with a 12-inch, describes it as a “large irregularly elliptical faintly luminous haze more than 5' across, with some faint stars involved. The centre, about 30 arc seconds wide, is bright and appears granular.” He notes that in good conditions, it is easily seen with a 4-inch telescope.

A 4-inch telescope shows it as a bright oval patch about 2' across, surrounded by a very faint glow. A 10-inch scope shows it as a large, oval halo of greenish nebulosity with a bright nuclear glow. On dark nights, the spiral structure of the halo is plainly visible. Several faint foreground stars can be seen in the halo. Larger telescopes show striking detail in the galaxy's arms, including several bright knots of nebulosity and a very obvious spiral pattern.

Sanford calls is a large barred spiral with a low surface brighteness. He notes that only the nuclear area is seen in smaller telescopes. A 10-inch shows the many HII regions and OB associations in the galaxy. The extent of the graceful arms may be traced by these small groupings for about 180 degrees in each arm, especially to the north of the nucleus.

ASV Journal Vol 24 No 3 June 1971: “just visible in 3-inch.”

Included in the CCD-atlas of Ryder S.D. & Dopita M.A. (1993) “An H-alpha Atlas of Nearby Southern Spiral Galaxies” Astrophys.J.Suppl. 88, 415. They note: “The delicate nature of its multitude of spiral arms make NGC 6744 one of the prettiest galaxies in the whole sky. Although it spans some 16’ in diameter, we felt it so worthy of inclusion in our atlas that we elected to attempt mosaicking. Three images, each overlapping the adjacent one by about 50 percent, have been registered and appropriately scaled in intensity in order to produce each of the mosaics, which cover a field of some 17.5’ x 10.3’. The vignetted corners of the component images have been masked out, and the hydrogen-alpha and red continuum images are presented separately to preserve a similar scale to the other images in this atlas.”

11x80: (exurban skies) A delicate nebulous presence with a 9.5m star north, not shown on the Uranometrias. Probably wouldn’t have seen it but for the chart’s precise position. (darker skies, seeing 6, transparency 7, darkness 7, lim mag naked eye, pole 6.0) “A faint presence, best seen with averted vision. Not round. Has a small star on its W-NW edge. An easy starhop from bright naked-eye stars.” (pristine skies, Sutherland, SAAO plateau) “Large, ghostly haze. Although easy once found, it remains a challenge because of its low surface brightness.” [AS]

8-inch Meade, 18mm eyepiece, 36.2’ fov: Faint, large, irregular galaxy with a sudden bright nucleus. Elongated (20 x 15) from north east to south west, with a hint of maybe very faint dust extended areas. One medium star proceeding to the northwest edge. [MS]

15.5-inch f/9 Newtonian: In a 15.5-inch telescope at 220x, the galaxy is clearly visible as an extended but faint, regular, elliptical patch. It looks somewhat like a small, faint globular cluster, as you see a bright, extended nucleus rapidly fading outwards. (suburban skies, light pollution) [AS]

NGC 6684
ESO104-G016, GCL-102
RA 18:48:56
Dec -65°10.4'
Galaxy

h: “B, R, psvmbM, 40 arcseconds, has a star 6-7 or 7m 5' or 6' N.p..” On a second occassion he called it “vB, R, first vg, then psmbM, 90 arcseconds, a star 6-7 m 7' S.p.”

This fine barred spiral lies close to the 6th magnitude Theta Pav. It shines at magnitude 10.5 and measures 4' by 3', appearing as a large oval halo of nebulosity with a bright, almost stellar nucleus.

Hartung describes this galaxy as round and symmetrical, about 45” across, rising sharply to an almost stellar nucleus. He notes that the “bright pale yellow Theta Pavonis is 6' Np and interferes with observation.” The galaxy is best observed on nights of good seeing when high magnification can be used to place the interfering star outside the field of view.

ASV Journal Vol 24 No 3 June 1971: “6' sf Theta Pav. Glimpsed in 4-inch.”

The RNGC (Sulentic and Tifft 1973) notes that this is a 11.5 mag globular cluster.

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"Deepsky Observers Companion" (http://www.global.co.za/~auke) Copyright 1998 Auke Slotegraaf. All rights reserved. Uranometria 2000.0 copyright (c) 1987-1996 Willmann-Bell, Inc. Page last updated 1998 March 01