U 367
11:00 to 11:40
-28° to -39°
Ant, Cen, Hya

FEATURED OBJECTS: NGC 3621 (Ben 46) , NGC 3742 , NGC 3557 , NGC 3717 , ESO378-PN001 .

NGC 3621
Bennett 46
ESO377-G037
RA 11:18:16
Dec -32° 48.8'
Gal

Discovered in 1790 by William Herschel (H I-241): "cB, E 70 degrees np-sf, vgbM, 7' long, 4' broad, within a parallelogram."

Dunlop 617: "a very faint pretty large nebula, about 2' broad and 4' long, very faint at the edges. The brightest and most condensed part is near the south following extremity; a small star is involved in the north preceding extremity, and there are two small stars near the south extremity, but not involved."

h: "pB, vL, oval, vgvlbM, resolvable, 5' long, 3' broad."

Hartung notes: “lying in a trapezium of four stars in good contrast with a scattered star field is this conspicuous hazy ellipse about 5’ x 3’ in pa 160 deg, rising to the centre broadly . . quite easy, though faint, with 7.5cm.”

Houston includes this galaxy in his Hydra Hysteria. He calls it a "big spiral galaxy about 10' diameter and 10th mag. It lies about 1.5 degrees east-southeast of a small triangle of 6th and 7th mag stars."

Steve Coe (1992, The Deep-Sky Observer, Webb Society, Issue 1) observing with a 17.5-inch f/4.5 at 100x notes: "B, L, elongated, much brighter in the middle, seen in finder and 10x50 binoculars, nice."

Tom Lorenzin: “10.6M; 5' x 2' extent; large featureless ellipse; !good supernova prospect!.”

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: “This is another comparatively poorly studied galaxy despite having a lagre angular size and abundance of H II regions. One prominent arm extends southward from the small bulge and carries some of the most luminous H II regions in this galaxy, but once again, there seems to be no counterpart on the opposite side.Most of the rest of the H-alpha emission comes from the next arm outwards. Rifts of dust criss-cross the disk, but at this moderate inclunation (about 67 degrees0, it does not seem likely that such dust could conceal any significant H II regions on the far side of the disk.”

Other names: “UA232,E377-37”. Inclination: (face-on, in degrees) 53 Total photoelectric blue mag 10.18 Total colour index .62 Logarithm of the angular diameter D25 (arcminutes) 2.09 Blue photographic magnitude 9.56 This galaxy is included in a sample of galaxies with velocity less than 500km/s with respect to the centroid of the Local Group. [Nearby Galaxies. Schmidt K.-H., Priebe A., Boller T. (Astron. Nachr. 314, 371 (1993))]

11x80: Picked up this bright galaxy readily. It appears mottled, showing the involvement of faint stars. It is readily seen as an elongated (cigar-shaped) patch, which grows with averted vision. (suburban skies) [AS]

NGC 3742
MCG-06-26-001
RA 11:35:26
Dec -37° 55.6'
Gal

h: "pB, pL, R, glbM, 40 arcseconds." On a second occassion he called it "F, lE, gbM."

NGC 3557
MCG-06-25-005
RA 11:09:57
Dec -37° 32.3'
Gal

h: "pretty bright, small, round, brighter in the middle." On a second occassion he called it "very bright, round, pretty gradually much brighter in the middle, 30 arcseconds across, the first of a group of three." The other objects involved are NGC 3564 & NGC 3568.

Gerd Bahr-Vollrath (Noosa Heads, Queensland, Australia) writes in the The Webb Society Nebulae and Clusters Section Report No. 11, January 1993: "A close pair [NGC 3557 & NGC 3564] of faint and small galaxies. NGC 3557 is the brighter galaxy, to the west, and appears as a round, indistinct glow. NGC 3564 is considerably fainter and is only a soft, faint glow. (8-inch f/12 SCT)"

Sandage (1975, Astrophysical Journal, 202, 563-582) notes that this galaxy is a member of the NGC 3557 Group. Members include NGC 3557, NGC 3557B, NGC 3564, NGC 3568. Shobbrook (1966, Mon. Not. R. astr. Soc., Vol 131, p351-363) notes that this field galaxy to the Dorado Cluster has V = 10.97, B-V = 0.98 and U-B = 0.60. It measures 1.75 by 1.1.

NGC 3717
ESO439-G015
RA 11:31:30
Dec -30° 18.4'
Gal

h: "pF, S, mE, attached like a wisp to a star 13th mag." On a second occassion he called it "pB, S, mE, attached to a star."

Houston included this galaxy in his Hydra Hysteria. He calls it a "routine spiral about 5' long and 1' wide." He notes that both NGC 3673 and NGC 3717 are of similar brightness, although their discoverer, Sir John Herschel, called the former 'faint' and the latter 'pretty bright.'

Steve Coe (1992, The Deep-Sky Observer, Webb Society, Issue 1) observing with a 17.5-inch f/4.5 at 100x notes: "pB, S, elongated, star in north arm."

ESO378-PN001
PK283+25.01, VKDA 1
RA 11:26:42
Dec -34° 40.8'
Pln

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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 April 05