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Zoology and wildlife conservation

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Abstracts » Zoology and wildlife conservation

A dark cluster of galaxies at redshift z=1

Article Abstract:

Scientists have identified a far-off source of X-rays from the lensed quasi-stellar object labelled MG2016 + 112 (refs 1,2). The emission is like that of galaxy clusters elsewhere in the space region because they contain thermal bremsstrahlung radiation from a hot metal-rich, diffuse gaseous halo. The X-ray galaxy cluster may contain astronomical objects which have never been seen before, indicating that the theoretical description of metal enrichment process in galaxy clusters needs to be reviewed.

Author: Tamura, T., Hattori, M., Ikebe, Y., Asaoka, I., Takeshima, T., Bohringer, H., Mihara, T., Neumann, D.M., Schindler, S., Tsuru, T.
Publisher: Macmillan Publishing Ltd.
Publication Name: Nature
Subject: Zoology and wildlife conservation
ISSN: 0028-0836
Year: 1997
Discovery and exploration, Outer space, Space exploration, X-ray astronomy

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Discovery of a hierarchical distribution of dark matter in the Fornax cluster of galaxies

Article Abstract:

X-ray observations were conducted on gas found in the Fornax cluster of galaxies. The X-ray satellite Advanced Satellite for Cosmology and Astrophysics provided high-quality data. Dark matter was found to be distributed on at least two distinct length scales, one of the dominant central galaxy and the other of the cluster as a whole. The results indicate the existence of a hierarchy in dark matter distribution.

Author: Kikuchi, K., Tamura, T., Takahashi, T., Ikebe, Y., Ezawa, H., Fukazawa, Y., Hirayama, M., Ishisaki, Y., Kubo, H., Makishima, K., Matsushita, K., Ohashi, T.
Publisher: Macmillan Publishing Ltd.
Publication Name: Nature
Subject: Zoology and wildlife conservation
ISSN: 0028-0836
Year: 1996
Dark matter (Astronomy)

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A population of faint galaxies that contribute to the cosmic X-ray background

Article Abstract:

A survey was undertaken that was a 100 times more sensitive than previous studies n the 2-10 keV band. Many faint resolved sources were found with integrate flux accounting for 30% of the X-ray background int he range. The average spectrum of the resolved source is harder than nearby bright active galactic nuclei and near to the spectrum of the X-ray background radiation.

Author: Takahashi, T., Yamada, T., Inoue, H., Ohta, K., Ishisaki, Y., Makishima, K., Ueda, Y., Akiyama, M., Tsuru, T., Sakano, M., Ogasaka, Y.
Publisher: Macmillan Publishing Ltd.
Publication Name: Nature
Subject: Zoology and wildlife conservation
ISSN: 0028-0836
Year: 1998
X-rays, X-ray diffraction, Electromagnetic scattering

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Subjects list: Research, Galaxies, Galaxy clusters
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