FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2268553864> ?p ?o ?g. }

• W2268553864 endingPage "77" @default.
• W2268553864 startingPage "77" @default.
• W2268553864 abstract "In our previous works, we found absorbed thermal X-ray plasma with kT 0.3 keV observed ubiquitously near the edges of the Fermi bubbles and interpreted this emission as weakly shock-heated Galactic halo gas. Here we present a systematic and uniform analysis of archival Suzaku (29 pointings; 6 newly presented) and Swift (68 pointings; 49 newly presented) data within Galactic longitudes < 20° and latitude 5°≲ < 60°, covering the whole extent of the Fermi bubbles. We show that the plasma temperature is constant at kT 0.30 ± 0.07 keV, while the emission measure (EM) varies by an order of magnitude, increasing toward the Galactic center (i.e., low ) with enhancements at the North Polar Spur (NPS), SE-claw, and NW-clump features. Moreover, the EM distribution of kT 0.30 keV plasma is highly asymmetric in the northern and southern bubbles. Although the association of the X-ray emission with the bubbles is not conclusive, we compare the observed EM properties with simple models assuming (i) a filled halo without bubbles, whose gas density follows a hydrostatic isothermal model (King profile), and (ii) a bubble-in-halo in which two identical bubbles expand into the halo, forming thick shells of swept halo gas. We argue that the EM profile in the north (b > 0°) favors (ii), whereas that of the south (b < 0°) is rather close to (i), but a weak excess signature is clearly detected also in the south like NPS (South Polar Spur). Such an asymmetry, if due to the bubbles, cannot be fully understood only by the inclination of bubbles' axis against the Galactic disk normal, thus suggesting asymmetric outflow due to different environmental/initial conditions." @default.
• W2268553864 created "2016-06-24" @default.
• W2268553864 creator A5017906960 @default.
• W2268553864 creator A5058309297 @default.
• W2268553864 creator A5066956730 @default.
• W2268553864 creator A5067366452 @default.
• W2268553864 creator A5068607244 @default.
• W2268553864 creator A5078738067 @default.
• W2268553864 creator A5090380354 @default.
• W2268553864 date "2015-07-01" @default.
• W2268553864 modified "2023-10-02" @default.
• W2268553864 title "GLOBAL STRUCTURE OF ISOTHERMAL DIFFUSE X-RAY EMISSION ALONG THE FERMI BUBBLES" @default.
• W2268553864 cites W1891457057 @default.
• W2268553864 cites W1964672324 @default.
• W2268553864 cites W1978316006 @default.
• W2268553864 cites W1980231566 @default.
• W2268553864 cites W1989617464 @default.
• W2268553864 cites W1996758820 @default.
• W2268553864 cites W1996932215 @default.
• W2268553864 cites W2005969899 @default.
• W2268553864 cites W2009082673 @default.
• W2268553864 cites W2016623635 @default.
• W2268553864 cites W2016888075 @default.
• W2268553864 cites W2023693056 @default.
• W2268553864 cites W2027993584 @default.
• W2268553864 cites W2032156227 @default.
• W2268553864 cites W2032372224 @default.
• W2268553864 cites W2037790414 @default.
• W2268553864 cites W2039797267 @default.
• W2268553864 cites W2041661662 @default.
• W2268553864 cites W2043629657 @default.
• W2268553864 cites W2043840829 @default.
• W2268553864 cites W2044062140 @default.
• W2268553864 cites W2044979165 @default.
• W2268553864 cites W2046191203 @default.
• W2268553864 cites W2050914817 @default.
• W2268553864 cites W2052926897 @default.
• W2268553864 cites W2069202754 @default.
• W2268553864 cites W2079692712 @default.
• W2268553864 cites W2091568451 @default.
• W2268553864 cites W2093210132 @default.
• W2268553864 cites W2101466017 @default.
• W2268553864 cites W2106574846 @default.
• W2268553864 cites W2126271344 @default.
• W2268553864 cites W2128323490 @default.
• W2268553864 cites W2129996269 @default.
• W2268553864 cites W2130101183 @default.
• W2268553864 cites W2134413610 @default.
• W2268553864 cites W2140317184 @default.
• W2268553864 cites W2154829343 @default.
• W2268553864 cites W2159179033 @default.
• W2268553864 cites W2165063682 @default.
• W2268553864 cites W2194080530 @default.
• W2268553864 cites W2796705535 @default.
• W2268553864 cites W3098035854 @default.
• W2268553864 cites W3098464313 @default.
• W2268553864 cites W3099966559 @default.
• W2268553864 cites W3100317759 @default.
• W2268553864 cites W3100537080 @default.
• W2268553864 cites W3100609337 @default.
• W2268553864 cites W3101500330 @default.
• W2268553864 cites W3101539948 @default.
• W2268553864 cites W3101823059 @default.
• W2268553864 cites W3101937814 @default.
• W2268553864 cites W3104139193 @default.
• W2268553864 cites W3104435135 @default.
• W2268553864 cites W3104812539 @default.
• W2268553864 cites W3105267595 @default.
• W2268553864 cites W4294947872 @default.
• W2268553864 doi "https://doi.org/10.1088/0004-637x/807/1/77" @default.
• W2268553864 hasPublicationYear "2015" @default.
• W2268553864 type Work @default.
• W2268553864 sameAs 2268553864 @default.
• W2268553864 citedByCount "33" @default.
• W2268553864 countsByYear W22685538642015 @default.
• W2268553864 countsByYear W22685538642016 @default.
• W2268553864 countsByYear W22685538642017 @default.
• W2268553864 countsByYear W22685538642018 @default.
• W2268553864 countsByYear W22685538642019 @default.
• W2268553864 countsByYear W22685538642020 @default.
• W2268553864 countsByYear W22685538642021 @default.
• W2268553864 countsByYear W22685538642022 @default.
• W2268553864 countsByYear W22685538642023 @default.
• W2268553864 crossrefType "journal-article" @default.
• W2268553864 hasAuthorship W2268553864A5017906960 @default.
• W2268553864 hasAuthorship W2268553864A5058309297 @default.
• W2268553864 hasAuthorship W2268553864A5066956730 @default.
• W2268553864 hasAuthorship W2268553864A5067366452 @default.
• W2268553864 hasAuthorship W2268553864A5068607244 @default.
• W2268553864 hasAuthorship W2268553864A5078738067 @default.
• W2268553864 hasAuthorship W2268553864A5090380354 @default.
• W2268553864 hasConcept C121332964 @default.
• W2268553864 hasConcept C1276947 @default.
• W2268553864 hasConcept C132552067 @default.
• W2268553864 hasConcept C134853933 @default.
• W2268553864 hasConcept C145148216 @default.
• W2268553864 hasConcept C184665706 @default.
• W2268553864 hasConcept C185544564 @default.

• next