This is an 15.0 minute exposure with
an STL-1301E CCD camera thru Kopernik's 20-inch F/8.1 Ritchey Chretien
Cassegrain telescope taken on April 10, 2005 at 5:50 UT. The field of view
is 22x22 arc minutes with North at the top.
NGC 5468 and NGC 5472 are a pair of Spiral Galaxies in the Constellation of Virgo. They have similar red shifts and therefore they are probably close to each other, but they are not interacting.
NGC 5468: This galaxy has a small bright nucleus and perhaps a short bar. There are two thin principal arms that can be followed from the center outward, one for half a revolution and the other for a quarter revolution, before they branch into several thin fragments winding through the outer disk. The resulting arm pattern is open. Although the arms are multiple, they remain thin and do not cover a large area of the outer disk.
NGC 5472: NGC 5472 has a small, bright, elongated nucleus that is not in the center of a bright lens shaped body. It is probably an edge-on spiral galaxy.
Non-existent NGC/IC Objects in this field: NGC 5467 = IC 973 and NGC 5465 = IC 974. They are both stars south of NGC 5468, and not galaxies. They were found by Bigourdan while he was trying to recover the three "nebulae" supposedly seen by Tempel near NGC 5468. Bigourdan somehow became a bit confused by the field, so did not realize immediately that one of his "novae" (IC 973) was the same star that he took to be NGC 5467. He published it in his first "Comptes Rendus" list, so it got an IC number. He caught the erroneous identity later when he was preparing his complete observations for publication.
Classification: SAB(rs)cd Dreyer description in the NGC: |
Classification: : SA(r)ab? sp Dreyer description in the NGC:
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George Normandin, KAS
April 19th, 2005