This is an 20 minute exposure with an
ST-9E CCD camera thru Kopernik's 20-inch F/8.1 Ritchey Chretien Cassegrain
telescope taken on June 24, 2004 centered at 3:00 UT. The RGB color exposures
were 10 minutes each. The field of view is 8x8 arc minutes with North at
the top.
NGC 4568 & NGC 4567:
This pair of Spiral Galaxies in Virgo is known as "The Siamese Twins" or "The Butterfly Galaxies". Both are classic spiral galaxies with small bright nuclei, several knotty arms, and arm segments. Both also have a hint of an inner ring. The pair is probably a member of the Virgo Galaxy Cluster. NGC 4568 is currently the host galaxy of Supernova 2004cc (Type Ic) and was also the host of Supernova 1990B a Type Ic that reached a maximum magnitude of 14.4.
Since they both have nearly the same red shift they may well be very close or in actual contract. However, other than a dim general x-ray glow involving both galaxies there is no indication of interaction. Neither galaxy is distorted nor are there any tidal tails. If they are in contract their orbital dynamics is such that they have not become distorted. Based on their red shifts they are roughly 120 million light years away (Hubble Constant of 62 Km per sec., per Megaparsec) and at that distance the projected distance between their nuclei is only 45,200 light years.
Classification: SA(rs)bc Dreyer description in the NGC: |
Classification: SA(rs)bc Dreyer description in the NGC:
|
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George Normandin, KAS
June 29th, 2004