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・ NGC 2119
・ NGC 2129
・ NGC 2146
・ NGC 2158
・ NGC 2169
・ NGC 2170
・ NGC 2174
・ NGC 2175
・ NGC 22
・ NGC 2204
・ NGC 2207 and IC 2163
・ NGC 2217
・ NGC 2232
・ NGC 2240
・ NGC 1090
NGC 1097
・ NGC 11
・ NGC 110
・ NGC 111
・ NGC 112
・ NGC 1128
・ NGC 113
・ NGC 1134
・ NGC 114
・ NGC 115
・ NGC 1156
・ NGC 116
・ NGC 1169
・ NGC 117
・ NGC 118


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NGC 1097 : ウィキペディア英語版
NGC 1097

NGC 1097 is a barred spiral galaxy about 45 million light-travel years away in the constellation Fornax. It was discovered by William Herschel on 9 October 1790. It is a severely interacting galaxy with obvious tidal debris and distortions caused by interaction with the companion galaxy NGC 1097A. Three supernovae (SN 1992bd, SN 1999eu, and SN 2003B) have been observed in NGC 1097 since 1992.
==General information==
NGC 1097 is also a Seyfert galaxy. Deep photographs revealed four narrow optical jets that appear to emanate from the nucleus. These have been interpreted as manifestations of the (currently weak) active nucleus. Subsequent analysis of the brightest jet's radio-to-X-ray spectral energy distribution were able to rule out synchrotron and thermal free-free emission. The optical jets are in fact composed of stars. The failure to detect atomic hydrogen gas in the jets (under the assumption that they were an example of tidal tails) using deep 21 cm HI imaging with the Very Large Array radio telescope and numerical simulations led to the current interpretation that the jets are actually the shattered remains of a cannibalized dwarf galaxy.
NGC 1097 has a supermassive black hole at its center, which is 140 million times the mass of the Sun. Around the central black hole is a glowing ring of star-forming regions with a network of gas and dust that spirals from the ring to the black hole. An inflow of material toward the central bar of the galaxy causes new stars to be created in the ring. The ring is approximately 5,000 light-years in diameter, the spiral arms of the galaxy extend tens of thousands of light-years beyond the ring.〔
NGC 1097 has two satellite galaxies, NGC 1097A and NGC 1097B. Dwarf elliptical galaxy NGC 1097A is the larger of the two. It is a peculiar elliptical galaxy that orbits 42,000 light-years from the center of NGC 1097. Dwarf galaxy NGC 1097B (5 x 106 solar masses), the outermost one, was discovered by its HI emission, and appears to be a typical dwarf irregular. Little else is known about it.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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