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Going Deep<br />

4923<br />

4921<br />

4919<br />

PGC 44864<br />

4907<br />

IC 4045<br />

4908<br />

IC 4051<br />

4911<br />

62 May 2012 sky & telescope<br />

PGC 44784<br />

IC 4040<br />

IC 4041<br />

IC 4042<br />

4906<br />

4895<br />

4889<br />

4881<br />

4883<br />

4874<br />

4865<br />

4860<br />

IC 3955<br />

This photograph from the Sloan Digital Sky Survey includes all the galaxies described by the author. Labels in the central region<br />

are omitted for clarity; see the close-up on the facing page for full details.<br />

galaxies, so its core h<strong>as</strong> a higher surface brightness. It<br />

also h<strong>as</strong> a faint nucleus. Small<br />

IC 4045 completes the line. I could fi nd ghostly IC 4040<br />

only because it makes an equilateral triangle with NGC<br />

4908 and IC 4045.<br />

The Cluster’s Heart<br />

The giant elliptical galaxy NGC 4889 appears signifi -<br />

cantly brighter than its binary companion, NGC 4874.<br />

At 229× NGC 4889 is slightly elongated e<strong>as</strong>t to west, and<br />

strongly concentrated in the center, with a prominent<br />

nucleus. Round NGC 4874 is very gradually concentrated<br />

to a fairly faint nucleus.<br />

What I fi nd particularly interesting are the tiny satellite<br />

galaxies in tight orbits around the two giants —presumbably<br />

on their way to becoming lunch! NGC 4874 h<strong>as</strong><br />

three very close companions visible in the 16-inch, NGC<br />

4871, NGC 4872, and NGC 4873. It also h<strong>as</strong> a host of<br />

PGC galaxies swarming around it that I look forward to<br />

attempting with a bigger scope. It took me several tries to<br />

4869<br />

4864<br />

4867<br />

4858<br />

unveil tough IC 3998, which lies between the two giants.<br />

NGC 4889 h<strong>as</strong> two very obvious companions at 229×,<br />

NGC 4886 and NGC 4898, and two challenging ones,<br />

15th-magnitude NGC 4894 and IC 4011. The latter<br />

two were made e<strong>as</strong>ier to fi nd by their proximity to the<br />

brighter galaxies.<br />

In contr<strong>as</strong>t, there’s no nearby landmark pointing the<br />

way to 14.4-magnitude NGC 4883, which hides 4′ northwest<br />

of NGC 4889 in the troublesome glare of the nearby<br />

7th-magnitude star.<br />

NGC 4876 is 3′ southe<strong>as</strong>t of NGC 4874’s nucleus.<br />

Once I found NGC 4876, I could intermittently see very<br />

small, faint NGC 4875 between the two signifi cantly<br />

e<strong>as</strong>ier 14th-magnitude galaxies that fl ank it, NGC 4876<br />

and IC 3973. It’s surprising that Guillaume Bigourdan,<br />

who discovered NGC 4875, missed the much e<strong>as</strong>ier IC<br />

galaxy only 2′ southwest.<br />

The Western End — and Beyond<br />

Slightly elongated NGC 4869 is e<strong>as</strong>y, <strong>as</strong> is NGC 4864.<br />

10’<br />

PGC 44467

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