The first picture below identifies Supernova 2001 ib (in NGC 7242), while the second identifies the members of this Galaxy Cluster.
These images are a mosaic of two 10
minute exposures with an ST-9E CCD camera thru Kopernik's 20-inch F/8.1
Ritchey Chretien Cassegrain telescope taken on December 12th, 2001 at 0:20
UT.
This group of 9 galaxies in the constellation of Lacerta forms the WBL 679 Galaxy Cluster. The two dominant galaxies are NGC 7242, an Elliptical Galaxy with a close companion, and NGC 7040, a Lenticular Galaxy. The remaining galaxies are all elliptical or lenticular types, with the exception of Spiral Galaxy IC 1441. All of these galaxies have about the same red shift and therefore all are probably true cluster members. There is some confusion as to the identification of the galaxies in this cluster that are included in the Index Catalog (IC), since the discoverer only provided Dreyer descriptions, but not the positions.
Classification: Elliptical (uncertain) |
Classification: Lenticular (uncertain) |
Classification: Elliptical (companion of NGC 7242) |
Classification: Elliptical (uncertain) |
Classification: Spiral |
Classification: Elliptical (uncertain) |
Classification: Lenticular |
Classification: Lenticular |
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George Normandin, KAS
December 14th, 2001