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Perseus constellation / Light sources / Plasma physics / NGC / Galaxy filament / Perseus Cluster / Corona / Protostar / Star / Astronomy / Extragalactic astronomy / Space


Embargoed until 19:00 (CEST)/1.00pm (EDT) 20 August, 2008. Magnetic support of the optical emission line filaments in NGC 1275 A. C. Fabian1, R. M. Johnstone1, J. S. Sanders1, C. J. Conselice2, C. S. Crawford1, J. S. Gal
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Document Date: 2008-08-11 08:33:26


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File Size: 2,28 MB

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City

Berlin / San Francisco / Tucson / Cambridge / Nottingham / /

Company

Fruchter A. S. / Reuland / Hatch N. A. / Astronomical Data Analysis Software / /

Country

United States / United Kingdom / /

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Facility

Space Telescope Science Institute / University of Arizona Press / Institute of Astronomy / centre of NGC / University of Wisconsin / /

IndustryTerm

neural network / gas mass / online version / intracluster gas / cold gas / molecular gas / imaging / hot gas / energy / /

Organization

Institute of Astronomy / School of Physics & Astronomy / National Aeronautics and Space Administration / Space Telescope Science Institute / University of Arizona Press / University of Wisconsin / Madison / Royal Society / Astronomical Society of the Pacific / /

Person

Hook / /

Position

R. N. / Author information Reprints / model for the smooth galactic light / /

ProvinceOrState

Wisconsin / /

PublishedMedium

Solar Physics / /

Technology

X-ray / neural network / /

URL

www.nature.com/nature / /

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