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Extragalactic astronomy / Supermassive black hole / Spiral galaxy / Black hole / Bulge / Dark matter / Galaxy formation and evolution / José Gabriel Funes / Astronomy / Physics / Galaxies


an immense amount of radiation. Once beyond the event horizon, this gas can no longer be seen. However, it does add to the mass of the black hole. This is a major way by which black holes grow, but as
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Document Date: 2011-08-29 03:38:09


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City

Baltimore / /

Company

NASA/Jet Propulsion Laboratory / /

Country

United States / /

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Facility

Planck Institute / Center (CXC)/Max Planck Institute / University of Arizona/C. Engelbracht / reTelescope Science Institute / Johns Hopkins University / Max Planck Institute / /

IndustryTerm

cold dense gas / halo gas / satellite systems / star considerable energy / jet travel / hot and tenuous gas / food source / dense gas / fresh gas / hot tenuous gas / little energy / cold gas / still accreting gas axy / cold gas galaxies / gas traveling / imaging / gas fractions / hot gas / nearby gas clouds / cooler gas / gas atmospheres surrounding / food / energy / /

Organization

reTelescope Science Institute / Center for Astrophysical Sciences / Association of Universities for Research / Max Planck Institute for Extraterrestrial Physics / National Science Foundation / NASA’s NuStar mission / US Federal Reserve / Max Planck Institute / National Aeronautics and Space Administration / Johns Hopkins University / Department of Physics However / 2Max Planck Institute for Astrophysics / University of Arizona / /

Person

B. R. McNamara / /

ProvinceOrState

Arizona / /

RadioStation

Radio Astronomy Observa / /

Technology

radiation / x-ray / spectroscopy / ESA / /

URL

http /

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