FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2221796744> ?p ?o ?g. }

• W2221796744 endingPage "94" @default.
• W2221796744 startingPage "94" @default.
• W2221796744 abstract "We present the first sub-arcminute images of the Galactic Center above 10 keV, obtained with NuSTAR. NuSTAR resolves the hard X-ray source IGR J17456–2901 into non-thermal X-ray filaments, molecular clouds, point sources, and a previously unknown central component of hard X-ray emission (CHXE). NuSTAR detects four non-thermal X-ray filaments, extending the detection of their power-law spectra with Γ ∼ 1.3–2.3 up to ∼50 keV. A morphological and spectral study of the filaments suggests that their origin may be heterogeneous, where previous studies suggested a common origin in young pulsar wind nebulae (PWNe). NuSTAR detects non-thermal X-ray continuum emission spatially correlated with the 6.4 keV Fe Kα fluorescence line emission associated with two Sgr A molecular clouds: MC1 and the Bridge. Broadband X-ray spectral analysis with a Monte-Carlo based X-ray reflection model self-consistently determined their intrinsic column density (∼1023 cm−2), primary X-ray spectra (power-laws with Γ ∼ 2) and set a lower limit of the X-ray luminosity of Sgr A* flare illuminating the Sgr A clouds to LX ≳ 1038 erg s−1. Above ∼20 keV, hard X-ray emission in the central 10 pc region around Sgr A* consists of the candidate PWN G359.95–0.04 and the CHXE, possibly resulting from an unresolved population of massive CVs with white dwarf masses MWD ∼ 0.9 M⊙. Spectral energy distribution analysis suggests that G359.95–0.04 is likely the hard X-ray counterpart of the ultra-high gamma-ray source HESS J1745–290, strongly favoring a leptonic origin of the GC TeV emission." @default.
• W2221796744 created "2016-06-24" @default.
• W2221796744 creator A5004495261 @default.
• W2221796744 creator A5010524716 @default.
• W2221796744 creator A5011270437 @default.
• W2221796744 creator A5015998182 @default.
• W2221796744 creator A5017623015 @default.
• W2221796744 creator A5018324841 @default.
• W2221796744 creator A5022157558 @default.
• W2221796744 creator A5025169326 @default.
• W2221796744 creator A5025718836 @default.
• W2221796744 creator A5027577812 @default.
• W2221796744 creator A5028255329 @default.
• W2221796744 creator A5030243019 @default.
• W2221796744 creator A5030771447 @default.
• W2221796744 creator A5034427738 @default.
• W2221796744 creator A5039553136 @default.
• W2221796744 creator A5040747406 @default.
• W2221796744 creator A5042527463 @default.
• W2221796744 creator A5043540900 @default.
• W2221796744 creator A5050667784 @default.
• W2221796744 creator A5054070152 @default.
• W2221796744 creator A5055583239 @default.
• W2221796744 creator A5056536327 @default.
• W2221796744 creator A5061339144 @default.
• W2221796744 creator A5062928530 @default.
• W2221796744 creator A5063948831 @default.
• W2221796744 creator A5068285125 @default.
• W2221796744 creator A5069726207 @default.
• W2221796744 creator A5076153543 @default.
• W2221796744 creator A5077160601 @default.
• W2221796744 creator A5078330440 @default.
• W2221796744 creator A5078330978 @default.
• W2221796744 creator A5080299919 @default.
• W2221796744 creator A5082652920 @default.
• W2221796744 creator A5082749953 @default.
• W2221796744 creator A5082924617 @default.
• W2221796744 creator A5083512039 @default.
• W2221796744 creator A5087174718 @default.
• W2221796744 creator A5087351960 @default.
• W2221796744 date "2015-11-19" @default.
• W2221796744 modified "2023-10-14" @default.
• W2221796744 title "<i>NuSTAR</i>HARD X-RAY SURVEY OF THE GALACTIC CENTER REGION. I. HARD X-RAY MORPHOLOGY AND SPECTROSCOPY OF THE DIFFUSE EMISSION" @default.
• W2221796744 cites W1498637236 @default.
• W2221796744 cites W1630568740 @default.
• W2221796744 cites W1841419560 @default.
• W2221796744 cites W1844333606 @default.
• W2221796744 cites W1964542248 @default.
• W2221796744 cites W1969536390 @default.
• W2221796744 cites W1974814479 @default.
• W2221796744 cites W1977426109 @default.
• W2221796744 cites W1979081980 @default.
• W2221796744 cites W1980527999 @default.
• W2221796744 cites W1983258465 @default.
• W2221796744 cites W1983480654 @default.
• W2221796744 cites W1984008682 @default.
• W2221796744 cites W1985551965 @default.
• W2221796744 cites W1994117136 @default.
• W2221796744 cites W1994292283 @default.
• W2221796744 cites W1997735880 @default.
• W2221796744 cites W2001182695 @default.
• W2221796744 cites W2002483171 @default.
• W2221796744 cites W2003209192 @default.
• W2221796744 cites W2009082673 @default.
• W2221796744 cites W2012135418 @default.
• W2221796744 cites W2016787644 @default.
• W2221796744 cites W2017861944 @default.
• W2221796744 cites W2026818944 @default.
• W2221796744 cites W2027138324 @default.
• W2221796744 cites W2027488890 @default.
• W2221796744 cites W2029720434 @default.
• W2221796744 cites W2030867565 @default.
• W2221796744 cites W2032372224 @default.
• W2221796744 cites W2032401312 @default.
• W2221796744 cites W2032817371 @default.
• W2221796744 cites W2039258655 @default.
• W2221796744 cites W2044125088 @default.
• W2221796744 cites W2044990488 @default.
• W2221796744 cites W2046225530 @default.
• W2221796744 cites W2048206598 @default.
• W2221796744 cites W2049698372 @default.
• W2221796744 cites W2051162330 @default.
• W2221796744 cites W2054498796 @default.
• W2221796744 cites W2059551391 @default.
• W2221796744 cites W2061575248 @default.
• W2221796744 cites W2063212296 @default.
• W2221796744 cites W2064792020 @default.
• W2221796744 cites W2067869481 @default.
• W2221796744 cites W2071737814 @default.
• W2221796744 cites W2074347757 @default.
• W2221796744 cites W2078835499 @default.
• W2221796744 cites W2081542902 @default.
• W2221796744 cites W2081649326 @default.
• W2221796744 cites W2083405175 @default.
• W2221796744 cites W2084098739 @default.
• W2221796744 cites W2085427810 @default.
• W2221796744 cites W2086574988 @default.
• W2221796744 cites W2090194704 @default.

• next