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The Caldwell Objects

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100<br />

while performing this feat is a bonus.)<br />

From Hawaii 3rd-magnitude Lambda Centauri (a<br />

type B9II blue giant) is low, achieving an altitude<br />

of only 7° at upper culmination. Lambda<br />

Centauri has the same declination as Alpha (α)<br />

Crucis (Acrux), the southernmost star in the<br />

famous Southern Cross, and it can be found<br />

about 5½° west of it. Fortunately, the 4,200-foot<br />

summit of Kilauea offers a reasonably clear view<br />

of the southern Milky Way. Still, my views pale<br />

in comparison with those from the Southern<br />

Hemisphere, where the Centaurus Milky Way<br />

curdles into fluid folds of starlight high<br />

overhead.<br />

Lambda Centauri is easy to spot, being the<br />

brightest star roughly halfway between Acrux<br />

and the great Eta (η) Carinae Nebula (<strong>Caldwell</strong><br />

92). Seen on photographs, Lambda Centauri lies<br />

on the eastern rim of a conspicuous caldera of<br />

darkness that breaches the region's copious<br />

starclouds. To be sure you find Lambda Centauri<br />

in this star-rich region, start at Acrux and hop<br />

two naked-eye stars to the southwest. This will<br />

bring you to Eta Crucis,<br />

which is the easternmost<br />

star in a line of four<br />

equally spaced nakedeye<br />

stars (oriented<br />

southeast to northwest)<br />

ending at Lambda<br />

Centauri.<br />

To the naked eye, a<br />

dusty comet tail of light<br />

½° long flows from<br />

Lambda Centauri to the<br />

southeast. This glow<br />

emanates from an<br />

unresolved chain of a<br />

half dozen or so 7th- to<br />

8th-mag-nitude stars in<br />

Collinder 249. <strong>The</strong> view<br />

is<br />

much the same in 7x50 binoculars, though the<br />

star chain is well detached from Lambda<br />

Centauri. Under averted vision the chain<br />

transforms into a rectangle of scintillating<br />

starlight surrounded by a slight fog. Knowing<br />

that a nebula (IC 2948) surrounds this region, it is<br />

easy for me to assume that the glow comes from<br />

interstellar gas, but I could not convince myself<br />

of this from my Hawaii site; the glow, I feared,<br />

might also come from unresolved stars. <strong>The</strong><br />

emission nebula does pop out dramatically in<br />

many photographs of the region, such as that<br />

shown on page 397. In fact, some photographs<br />

suggest that IC 2948 rivals the nearby<br />

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

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