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The Caldwell Objects

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30<br />

but stars or at least to contain stars and to give<br />

"every other indication of consisting of stars<br />

entirely." With their modest instruments, today's<br />

amateurs can understand why Herschel made the<br />

assumptions he did. For example, when viewing<br />

NGC 7331 through a 6-inch telescope, Christian<br />

Luginbuhl and Brian Skiff detected a stellar<br />

nucleus and grainy texture within the disk.<br />

Increasing the aperture to 10 inches, they report,<br />

brought out increased mottling, especially in the<br />

inner halo, and two 13.5-magnitude stars west of<br />

the northern tip of the disk. Herschel, with his<br />

much larger instruments and very high<br />

magnifications, must have detected these<br />

features, among others, and he may well have<br />

envisioned something akin to a distant cluster,<br />

perhaps one like M4 in Scorpius, whose center is<br />

a needle of starlight.<br />

Through the Genesis at 23x NGC 7331 is<br />

wonderfully apparent as a small, elongated form<br />

nestled in a rich field of stars. With averted<br />

vision I perceive a tight lens-shaped core<br />

surrounded by a dim, elliptical outer halo or<br />

shell. At 72x and above, the galaxy becomes a<br />

complex mottled glow. Its nucleus appears<br />

especially sharp and is surrounded by fleeting<br />

120<br />

shadows of dust. My drawing shows a great<br />

amount of detail, which becomes visible over<br />

several hours of continuous observing. With time,<br />

the galaxy's mottled disk transforms into a clearly<br />

discernible spiral pattern with intermittent dust<br />

lanes, the most prominent being the western<br />

furrow. Most impressive, however, is that some of<br />

the mottling within the bright arms corresponds<br />

to true patches of stars or ΗII regions. One<br />

prominent region appears just northwest of an<br />

approximately 12th-mag-nitude star lying eastsoutheast<br />

of the lens-shaped core.<br />

NGC 7331 is haunted by several faint companions,<br />

four of which appear close to its western<br />

edge. I say haunted because, at 72x in the 4-inch,<br />

these companions seem to pop dimly into view<br />

with averted vision, only to vanish under a direct<br />

gaze. <strong>The</strong> brightest companion, NGC 7335, is<br />

listed in <strong>The</strong> Deep Sky Field Guide at magnitude<br />

13.3, though I wonder if it is not brighter; I blindly<br />

(and correctly) positioned the tiny fuzz ball in my<br />

original sketch, which I made at the eyepiece, and<br />

wondered in the margin if it was really a galaxy.<br />

Luginbuhl and Skiff detected two more<br />

companions, NGC 7337 (magnitude 14.4) and<br />

NGC 7340 (magnitude 13.7), with a 10-inch<br />

telescope. <strong>The</strong> fourth, NGC 7336, apparentiy was<br />

too difficult for them. <strong>The</strong> Deep Sky Field Guide lists<br />

it at magnitude 15.8, but Sky & Telescope's Roger<br />

W Sinnott . notes that this galaxy may not be so<br />

faint; the Lyon-Meudon Extragalactic Database, he<br />

says, attributes a blue magnitude of 15.4 to NGC<br />

7336, and it probably is a little brighter visually.<br />

About ½° south-southwest of NGC 7331,<br />

scrunched into a mere 3.5' of sky, are the five<br />

challenging galaxies collectively known as<br />

Stephan's Quintet: NGC 7317, NGC 7318A, NGC<br />

7318B, NGC 7319, and NGC 7320. Stephan's<br />

Quintet is of continual interest to astronomers. A<br />

1995 study shows that radio emission from<br />

Deep-Sky Companions: <strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong>

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