U 419
02:30 to 03:30
-39° to -50°
Ret, Eri, Hor
Oct-Feb

FEATURED OBJECTS: NGC 1031, ESO154-G023, NGC 1249, C0309-583, NGC 1252, NGC 1261, IC 1933.

NGC 1031
ESO154-G005
RA 02:36:38
Dec -54°51.6'
Galaxy

h: F, S, R, gbM, 20"; the following of two." The other object is NGC 1025.

Green, M. R. & Dixon, K. L. (1978) “Photoelectric photometry of bright southern galaxies”, Vol 98, August, p 167-169. They find the V magnitude through a 28’’ aperture = 13.39, and through a 80’’ aperture = 12.75.

ESO154-G023
Arp 255
RA 02:56:52
Dec -54°34.4'
Galaxy

NGC 1249
ESO155-G006
RA 03:10:02
Dec -53°20.1'
Galaxy

h: "bright; large; very much elongated in pos. 80 ; very gradually brighter in the middle to an axis; 2.5' long; 1' broad." He observed it some while later, writing: "Found in place and viewed p M, but very faintly seen."

De Vaucouleurs (1956) “Survey of bright galaxies south of -35° declination”, Mem. Mount Stromlo, No. 13. On photos taken with the 30-inch Reynolds reflector, 20-inch diaphragm: bright inner part 2.5’ x 1.3’, faint outer regions 4.8’ x 2.1’. Remarks: short bright bar, no BN, asymm.

C0309-583

RA 03:10:29
Dec -58°08.0'
Open cluster

NGC 1252

RA 03:10:29
Dec -58°08.0'
Open cluster?

h: Star 8th mag the chief of a cluster of 18 or 20 stars.

The RNGC (Sulentic and Tifft 1973) notes that this is a unverified southern object.

NGC 1261
GCL-5, ESO155-SC011
RA 03:12:14
Dec -55°13.0'
Globular cluster

Dunlop 337: "a very bright round nebula, about 1.5' diameter, pretty well defined and gradually bright to the centre. A small star north following."

h: "bright; large; irregularly round; 2.5' diameter; all resolved into equal stars 14mag. Has a star 9th mag 45 N.f. 3' distant." His second observation recorded it as "pretty bright; round; very gradually brighter in the middle; 3' across; resolved into stars of 15th magnitude. A very faint nebula (??) precedes."

Described in Union Obs. Circulars, 45-76, p 50. “Nebulae, clusters, etc. on Sydney Plates” as “Remarkable object; looks like a nebula on plates, but the images are poor, resolved into stars by h.

Hartung notes: “This well condensed globular cluste rlies in a fine field; 30cm resolves it into crowded stars right to the centre. It is about 2.5’ across and the scattered outliers do not extend far; the stars are however very faint and hard to detect with 20cm although the cluster looks granular. It is a fine bright object, conspicuous with 10.5cm.”

ASV Journal, Vol 24, No 3, June 1971: "many faint stars resolved in 12.5-inch 150x."

Van den Bergh and Hagen ("UBV photometry of star clusters in the Magellanic Clouds", Astronomical Journal, Vol. 73, 1968) find that the integrated V magnitude through a 60'' diaphragm is 9.61. They classify it as a globular cluster.

11x80: “Distinct smallish globular cluster, lies just south-west of a Triangulum Australis of stars. Close north-east is a 9th mag star, clearly separated, not touching as shown in Uranometrias. On edge of the binocular field lies the prominently red TW Hor.” (suburban skies, light and air pollution); “Part of a False Cross asterism. About 1.5 arc min across, 8.5 magnitude round glow. Small star off to the north-east. Look for the orange TW Hor due south. Rating: easy.” (suburban skies, seeing average-good); “A small, 45 arcsec, pretty bright cluster, like a softly focused small star. To the north-east, about 1 arcmin away, is a 9th magnitude star.” (exurban skies, seeing good) [AS]

IC 1933
ESO155-G025
RA 03:25:39
Dec -52°47.0'
Galaxy

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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