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The Caldwell Objects

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36<br />

This means that in shape NGC 4559 lies somewhere<br />

between a barred spiral and an unbarred<br />

one (SAB), whose inner arms form a ring that<br />

surrounds the needle-sharp nucleus (rs) while<br />

farther out the arms fly freely open (cd).<br />

Recent advances in our knowledge of the<br />

high-redshift universe are providing us with a<br />

better understanding of the history of galaxy<br />

morphology. For instance, the Hubble Space<br />

Telescope has shown that the distinction between<br />

ellipticals and spirals grows less definite with<br />

increasing distance, becoming nearly<br />

imperceptible in images that show how the<br />

universe looked when it was only one-tenth its<br />

current age. Other studies suggest that ellipticals<br />

formed remarkably early in the universe while<br />

spiral galaxies took much longer to form. <strong>The</strong><br />

origins and evolution of galaxy morphology<br />

remain active (and contentious) fields of research.<br />

NGC 4559 is a sizable galaxy, spanning<br />

100,000 light-years, with a total mass of 40 billion<br />

Suns. Together with NGC 4565 it is a member of<br />

the Coma-Sculptor Cloud of galaxies,<br />

140<br />

and it is receding from Earth at a speed of 820 km<br />

per second. <strong>The</strong> galaxy is inclined 69° from face<br />

on. In photographs NGC 4559 looks like a<br />

spinning saw blade whisking toward the observer<br />

at a skewed angle. Its untamed arms<br />

appear tormented, as if they have been stretched<br />

by three people in three different directions. <strong>The</strong><br />

arms are dotted with bright ΗII regions that seem<br />

to cling to them like lint to a sweater.<br />

In the mid-1990s the Rosat spacecraft<br />

revealed 17 discrete X-ray sources within NGC<br />

4559. <strong>The</strong> most luminous one, sited in the<br />

galaxy's nucleus, is slightly extended, suggesting<br />

either an unresolved superposition of several<br />

compact sources or a diffuse source of emission.<br />

Another bright source was found in an outlying<br />

spiral arm, where it coincides with a conspicuous<br />

group of Η II regions. Since little radio or infrared<br />

emission emerges from this location, the X-rays<br />

may have originated from a single, severalhundred-year-old<br />

supernova remnant.<br />

Small-telescope users will have no trouble<br />

locating NGC 4559. <strong>The</strong> galaxy lies only 2° eastsoutheast<br />

of magnitude-4.3 Gamma (γ)<br />

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

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