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The Caldwell Objects

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172<br />

42<br />

nent knot of stars lies to the south of the core. <strong>The</strong><br />

cluster is situated in a rich Milky Way field, so it<br />

is hard to discern which stars belong to the<br />

cluster and which to our galaxy's populous disk.<br />

Of course, with a really big telescope NGC<br />

7006 reveals itself in ways that can only be<br />

imagined by the owners of small instruments. In<br />

September 1998, Brent Archinal and I observed<br />

NGC 7006 with the 31-inch reflector at the<br />

Warren Rupp Observatory in Mansfield, Ohio.<br />

<strong>The</strong> cluster was a scintillating mass of dim<br />

starlight. At high power we saw an unresolved,<br />

starlike inner core surrounded by a dark ring that<br />

defined the inner edge of a finely resolved,<br />

though jagged, outer core. With averted vision<br />

thin arms radiated out from the stellar "hole" like<br />

the limbs of a starfish wrapped around a rock.<br />

<strong>The</strong> outer halo appeared loose and fractured, as if<br />

its shell were so old and brittle that pieces of it<br />

were flaking off into space.<br />

Large-telescope users might be interested in<br />

this challenge: a tiny cluster of galaxies lies just 5'<br />

to the southwest of NGC 7006. None of<br />

these galaxies is plotted on the Millennium Star<br />

Atlas, but a few of them can be seen in the<br />

Digitized Sky Survey image on page 169.I believe<br />

they will certainly fall to large Dobsonians.<br />

Before leaving the area be sure to return to<br />

Gamma Delphini, which is a beautiful double<br />

star. <strong>The</strong> magnitude-5.2 secondary lies 9" to the<br />

west of the yellowish primary; the stars were 12"<br />

apart in 1823. Adm. William Henry Smyth saw<br />

the secondary gleam with a "light emerald" hue.<br />

<strong>The</strong> colors Smyth saw recall those of the famous<br />

double star Albireo in the nose of Cygnus, the<br />

Swan. Interestingly, though, the spectral types of<br />

Gamma Delphini's components are K1IV<br />

(primary) and F7V (secondary), respectively —<br />

basically right next to each other on the<br />

OBAFGKM sequence of stellar spectral types. So<br />

any color contrast perceived by Smyth was<br />

undoubtedly due to psychology, or intensity<br />

threshold effects in the eye. I see two golden<br />

stars, with the fainter one having a cooler (bluer)<br />

hue. But the only important question is: what do<br />

you see?<br />

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

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