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The Caldwell Objects

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faintest of the five major members of the Sculptor<br />

Group, the detail it displays in small instruments<br />

makes it a superb, yet visually challenging, target<br />

for beginners. If we accept a distance of 9 million<br />

light-years for NGC 7793, its true linear diameter<br />

is 23,000 light-years. We see its disk inclined 50°<br />

from face on, so its tiny nuclear bulge and<br />

dominating spiral arms are prominendy<br />

revealed.<br />

15<br />

N G C 3 6 2 1<br />

T y S p e G i : a r l ( a S a l d x ) y<br />

C o H n y : d r a<br />

RA: 11 h 18.3 m<br />

Dec: -32° 49'<br />

Mag: 8.9<br />

SB: 12.9<br />

Dim: 14.9' x 7.4'<br />

Dist: 23 million light-years<br />

Hydra is host to innumerable galaxies, many of<br />

which can be picked up in small amateur<br />

instruments. Its biggest deep-sky prizes, of<br />

course, are M83, a magnificent spiral galaxy, and<br />

NGC 3242 (<strong>Caldwell</strong> 59), the Ghost of Jupiter<br />

planetary nebula. Spiral galaxy NGC 3621 is<br />

another bright denizen of Hydra, but very little<br />

attention has been paid to it. <strong>The</strong> galaxy is not<br />

included in many popular handbooks, though it<br />

is similar in size to M83 (albeit nearly 1½<br />

magnitudes fainter). In a 1993 Astrophysical<br />

Journal article NGC 3621 was referred to as<br />

"another comparatively poorly studied galaxy<br />

despite having a large angular size and<br />

abundance of ΗII regions." Once again, the low<br />

southerly declination and a lack of bright nearby<br />

stars may explain the neglect.<br />

To find NGC 3621 look 10° south and<br />

slightly east of Beta (β) Crateris and 3¼° west<br />

and slightly south of Xi (ξ) Hydrae. Tele-<br />

440<br />

scopically, the galaxy appears as a big diffuse<br />

glow with a bright core and a faint, elliptical halo.<br />

Its spiral arms are faint and will challenge smalltelescope<br />

users. <strong>The</strong> galaxy is reasonably large<br />

(100,000 light-years across) and the universe's<br />

expansion is carrying it away at a speed of 730<br />

km per second. In long-exposure photographs<br />

NGC 3621 is a remarkable pinwheel just 25° from<br />

edge on. Its small, bright nucleus is nestled in a<br />

bright ellipse of spiral arms (cut by rifts of dust)<br />

that gradually unwind into a fainter outer halo.<br />

One prominent arm extends southward from the<br />

small bulge; it carries some of this galaxy's most<br />

luminous ΗII regions.<br />

16<br />

N G C 1 3 4<br />

T y M p i e S x : p e G i d a r l ( a S x l A y B b c )<br />

C o S n c : u l p t o r<br />

RA: 00 h 30.4 m<br />

Dec: -33° 15'<br />

Mag: 10.4<br />

SB: 13.3<br />

Dim: 7.6' x 1.5'<br />

Dist: 62 million light-years<br />

NGC 134 is an extraordinary nearly edge-on<br />

spiral galaxy in Sculptor, which just happens to<br />

be surrounded by, and somewhat lost among, a<br />

cast of extragalactic prima donnas — namely<br />

NGC 253 (<strong>Caldwell</strong> 65), NGC 300 (<strong>Caldwell</strong> 70),<br />

and NGC 55 (<strong>Caldwell</strong> 72) — all of which are<br />

savagely beautiful galaxies for small telescopes.<br />

Nevertheless, NGC 134 is a treasure that's<br />

relatively easy to acquire. First locate 4thmagnitude<br />

Alpha (α) Sculptoris, which is some<br />

12° south-southeast of Deneb Kaitos, or Beta (β)<br />

Ceti. Next, use binoculars to locate 5thmagnitude<br />

Eta (η) Sculptoris about 7½°<br />

southwest of Alpha Sculptoris. Now center<br />

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

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