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The Caldwell Objects

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and kinked. All this detail is wrapped in a faint<br />

oval halo of light. At this power I see no welldefined<br />

spiral arms. With 130x and excellent<br />

seeing the northern clumps transform into a knot<br />

and a ribbon of nebulosity that curls gently<br />

eastward as part of the galaxy's feathery<br />

<strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong><br />

67<br />

inner spiral structure. A bright arc of light<br />

defines the northeastern edge of the outer lens,<br />

while an odd fuzzy patch to the southwest may<br />

be a dust-disturbed part of the nuclear region. Or<br />

is it a faint star?<br />

On the evening of December 30, 1996, I<br />

detected a very dim patch of light northwest of<br />

the main galaxy at high power. It was in the right<br />

position to have been NGC 1097A. But could I<br />

have seen that magnitude-13.6 companion galaxy<br />

in a 4-inch telescope? Quite possibly. Published<br />

galaxy magnitudes in this range are suspect.<br />

Christian Luginbuhl and Brian Skiff estimate<br />

NGC 1097A's visual magnitude to be around<br />

12.9, though I am certain it's probably a few<br />

tenths of a magnitude brighter. Comet hunters<br />

should note that the companion is not plotted on<br />

the Millennium Star Atlas, but it is in Uranometria<br />

2000.0.<br />

NGC 1097 is yet another <strong>Caldwell</strong> object for<br />

supernova hunters to keep an eye on. An HST<br />

image of NGC 1097 taken on September 30, 1992,<br />

captured Supernova 1992bd 12 days prior to its<br />

ground-based discovery 2" east and 9" south of<br />

the nucleus; the supernova shone at magnitude<br />

15 at the time of ground-based discovery. More<br />

recently, a magnitude-17.3 supernova appeared<br />

23" east and 157" south of the galaxy's center in<br />

November 1999.<br />

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