05.06.2013 Views

The Caldwell Objects

The Caldwell Objects

The Caldwell Objects

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

NGC 6231). Under averted vision the cluster<br />

appears to lie in the foreground of a galactic mist,<br />

an illusion caused by the faint glow of<br />

unresolved suns, many of which belong to the<br />

rich Milky Way background. Use high power and<br />

averted vision, and faint suns will peek out from<br />

the dark crevices between the brighter suns. If the<br />

arrowhead seems to visually sag to the east, it's<br />

because that's the densest part of the cluster, with<br />

a miniature assortment of some half dozen suns.<br />

Under high magnification many of the stars<br />

appear to be paired. <strong>The</strong><br />

two brightest suns marking the weapon's northern<br />

corner are themselves fine doubles; the<br />

northernmost of these two pairs shines at magnitude<br />

5.5 with a 7th-magnitude companion 65"<br />

away at a position angle of 13°.<br />

<strong>The</strong> cluster's radiance is magnified with even<br />

a slight increase in aperture. Through a 6-inch<br />

telescope Christian B. Luginbuhl and<br />

76<br />

Brian A. Skiff recorded 100 stars (not all cluster<br />

members) in a 10' area, and they saw many blue<br />

stars and small geometric patterns at low power.<br />

James Dunlop, who used a 9-inch reflector, saw a<br />

"cluster of pretty bright stars of mixt small<br />

magnitudes, considerably congregated to the<br />

centre, about 10' diameter, with a large branch of<br />

very small stars extended on the north side."<br />

With a 12-inch telescope Ernst Hartung spied<br />

"many bright white and yellow stars, and many<br />

pairs and triplets, which sparkle in patterns of<br />

lines and small groups." And with<br />

her 13.1-inch f/4.5 reflector<br />

Barbara Wilson recorded<br />

"eight brilliant white stars<br />

with dozens of fainter<br />

members in a very<br />

nebulous region" at the<br />

1986 Texas Star Party; the<br />

cluster's center, she noted,<br />

"has [a] dimmer streamer<br />

curving around it and a<br />

smaller streamer [to the]<br />

south."<br />

Do not stop with<br />

NGC 6231. <strong>The</strong> entire<br />

region is worth exploring.<br />

Certainly there is nothing<br />

like it in the entire sky for<br />

small-telescope users. Just<br />

north and east of the<br />

cluster, out to about 3°,<br />

are three open clusters<br />

(Trumpler 24, NGC 6242, and NGC 6268), a<br />

planetary nebula (IC 4637), a diffuse nebula (IC<br />

4628), double stars, colored stars, Milky Way<br />

patches, and a swath of dark nebulosity<br />

(Barnard 48). It's a cornucopia of celestial riches.<br />

IC 4628 lies at the northeastern end of Trumpler<br />

24, 1½° northeast of NGC 6231. It is an irregular<br />

90' x 60' patch of faintly glowing<br />

<strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong> 303

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!