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• W3100555438 endingPage "79" @default.
• W3100555438 startingPage "79" @default.
• W3100555438 abstract "Prior to the launch of NuSTAR, it was not feasible to spatially resolve the hard (E > 10 keV) emission from galaxies beyond the Local Group. The combined NuSTAR data set, comprised of three ∼165 ks observations, allows spatial characterization of the hard X-ray emission in the galaxy NGC 253 for the first time. As a follow up to our initial study of its nuclear region, we present the first results concerning the full galaxy from simultaneous NuSTAR, Chandra, and Very Long Baseline Array monitoring of the local starburst galaxy NGC 253. Above ∼10 keV, nearly all the emission is concentrated within 100'' of the galactic center, produced almost exclusively by three nuclear sources, an off-nuclear ultraluminous X-ray source (ULX), and a pulsar candidate that we identify for the first time in these observations. We detect 21 distinct sources in energy bands up to 25 keV, mostly consisting of intermediate state black hole X-ray binaries. The global X-ray emission of the galaxy—dominated by the off-nuclear ULX and nuclear sources, which are also likely ULXs—falls steeply (photon index ≳ 3) above 10 keV, consistent with other NuSTAR-observed ULXs, and no significant excess above the background is detected at E > 40 keV. We report upper limits on diffuse inverse Compton emission for a range of spatial models. For the most extended morphologies considered, these hard X-ray constraints disfavor a dominant inverse Compton component to explain the γ-ray emission detected with Fermi and H.E.S.S. If NGC 253 is typical of starburst galaxies at higher redshift, their contribution to the E > 10 keV cosmic X-ray background is <1%." @default.
• W3100555438 created "2020-11-23" @default.
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• W3100555438 date "2014-12-01" @default.
• W3100555438 modified "2023-10-01" @default.
• W3100555438 title "SPATIALLY RESOLVING A STARBURST GALAXY AT HARD X-RAY ENERGIES:<i>NuSTAR</i>,<i>CHANDRA</i>, AND VLBA OBSERVATIONS OF NGC 253" @default.
• W3100555438 cites W1963787353 @default.
• W3100555438 cites W1974047653 @default.
• W3100555438 cites W1974463200 @default.
• W3100555438 cites W1975634635 @default.
• W3100555438 cites W1981640818 @default.
• W3100555438 cites W1987319691 @default.
• W3100555438 cites W1992208355 @default.
• W3100555438 cites W2001955524 @default.
• W3100555438 cites W2002015260 @default.
• W3100555438 cites W2004088607 @default.
• W3100555438 cites W2016829940 @default.
• W3100555438 cites W2018910022 @default.
• W3100555438 cites W2021255107 @default.
• W3100555438 cites W2023237478 @default.
• W3100555438 cites W2034483141 @default.
• W3100555438 cites W2039866073 @default.
• W3100555438 cites W2041216266 @default.
• W3100555438 cites W2043469775 @default.
• W3100555438 cites W2045182435 @default.
• W3100555438 cites W2046211919 @default.
• W3100555438 cites W2048113312 @default.
• W3100555438 cites W2051770437 @default.
• W3100555438 cites W2051972472 @default.
• W3100555438 cites W2053852021 @default.
• W3100555438 cites W2055047616 @default.
• W3100555438 cites W2057011516 @default.
• W3100555438 cites W2060948490 @default.
• W3100555438 cites W2061225162 @default.
• W3100555438 cites W2066702849 @default.
• W3100555438 cites W2070451726 @default.
• W3100555438 cites W2074347757 @default.
• W3100555438 cites W2074408355 @default.
• W3100555438 cites W2076866511 @default.
• W3100555438 cites W2083852799 @default.
• W3100555438 cites W2085427810 @default.
• W3100555438 cites W2087449327 @default.
• W3100555438 cites W2089915781 @default.
• W3100555438 cites W2092007096 @default.
• W3100555438 cites W2096689909 @default.
• W3100555438 cites W2099255378 @default.
• W3100555438 cites W2107913129 @default.
• W3100555438 cites W2109222834 @default.
• W3100555438 cites W2112991723 @default.
• W3100555438 cites W2113112035 @default.
• W3100555438 cites W2116122188 @default.
• W3100555438 cites W2116996962 @default.
• W3100555438 cites W2117874169 @default.
• W3100555438 cites W2119439775 @default.
• W3100555438 cites W2127772312 @default.
• W3100555438 cites W2131939233 @default.
• W3100555438 cites W2135112604 @default.
• W3100555438 cites W2136262096 @default.
• W3100555438 cites W2137608234 @default.
• W3100555438 cites W2148139731 @default.
• W3100555438 cites W2151645158 @default.
• W3100555438 cites W2154509167 @default.
• W3100555438 cites W2162466104 @default.
• W3100555438 cites W2165265292 @default.
• W3100555438 cites W2170070152 @default.
• W3100555438 cites W2170454083 @default.
• W3100555438 cites W2323377960 @default.
• W3100555438 cites W3022520032 @default.
• W3100555438 cites W3098060678 @default.
• W3100555438 cites W3098105446 @default.
• W3100555438 cites W3098237314 @default.
• W3100555438 cites W3098259410 @default.
• W3100555438 cites W3098263962 @default.
• W3100555438 cites W3098578749 @default.
• W3100555438 cites W3099401213 @default.
• W3100555438 cites W3100040589 @default.
• W3100555438 cites W3100211458 @default.
• W3100555438 cites W3100534179 @default.
• W3100555438 cites W3100840462 @default.
• W3100555438 cites W3100886448 @default.

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