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The Caldwell Objects

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36<br />

NGC 4559<br />

Type: Mixed Spiral Galaxy (SABcd)<br />

Con: Coma Berenices<br />

RA: 12 h 36.0 m<br />

Dec: +27° 58'<br />

Mag: 10.0<br />

Dim: 11.3' x 5.0'<br />

SB: 14.3<br />

Dist: 32 million light-years<br />

Disc: William Herschel, 1785<br />

W. H ERSCHEL: [Observed 11 April<br />

1785] Very bright, very large, much<br />

extended from north preceding to<br />

south following [from northwest to<br />

southeast] 10' or 12' long. 4 stars in it.<br />

(Η I-92)<br />

GC/ NGC: Very bright, very large, much extended toward<br />

position angle 150°, gradually brighter in the middle, 3 stars<br />

following [to the east of the object].<br />

IN COMA BERENICES MORE THAN A DOZEN GAL-axies<br />

shine at 10th magnitude or brighter. Among<br />

these are the famous Black Eye Galaxy, M64, and<br />

the constellation's flagship spiral, NGC 4565<br />

(<strong>Caldwell</strong> 38), a textbook edge-on system. Just 2°<br />

due north of NGC 4565 (and perhaps overlooked<br />

because of its proximity to it) lies NGC 4559, a<br />

remarkable example of a spiral system in an<br />

intermediate morphological class.<br />

<strong>The</strong> galaxy classification scheme developed<br />

by Edwin P Hubble . in 1925 is simple enough.<br />

First it divides galaxies into three major types:<br />

ellipticals (E); unbarred spirals (S); and barred spirals<br />

(SB). Hubble's famous "tuning fork" diagram,<br />

which illustrated his galaxy types, also included<br />

a then-hypothetical transitional form of galaxy,<br />

which he dubbed simply "S0." S0, or lenticular,<br />

galaxies (since discov-<br />

<strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong><br />

36<br />

ered) are intermediate in form between ellipticals<br />

and spirals. <strong>The</strong>y are lens-shaped spheroids<br />

embedded in flattened disks that lack spiral<br />

structure. <strong>The</strong> unbarred and barred spiral families<br />

each branch off of the lenticular SO form on<br />

Hubble's diagram. Each branch is then subdivided<br />

largely according to the size of the<br />

galaxy's central bulge and the tightness of its<br />

spiral arms; both parameters are described by<br />

lowercase letters that range from "a" to "d". An<br />

"Sa" or "SBa" spiral has the largest nuclear region<br />

and most tightly wound arms, while an "Sd" or<br />

"SBd" spiral has the smallest nucleus and most<br />

loosely wound spiral arms.<br />

So where does NGC 4559 fit in? According<br />

to the so-called Revised Morphological Galaxy<br />

Classification System, an elaboration of Hubble's<br />

original scheme, the galaxy is a mixed SAB (rs)<br />

cd.<br />

139

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