FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3122889532> ?p ?o ?g. }

• W3122889532 endingPage "483" @default.
• W3122889532 startingPage "473" @default.
• W3122889532 abstract "We have analysed all the good quality XMM-Newton data publicly available for the bright ULXs Holmberg IX X-1 and NGC 1313 X-1, with the aim of searching for discrete emission or absorption features in the Fe K band that could provide observational evidence for the massive outflows predicted if these sources are accreting at substantially super-Eddington rates. We do not find statistically compelling evidence for any atomic lines, and the limits that are obtained have interesting consequences. Any features in the immediate Fe K energy band (6-7 keV) must have equivalent widths weaker than ~30 eV for Holmberg IX X-1, and weaker than ~50 eV for NGC 1313 X-1 (at 99 per cent confidence). In comparison to the sub-Eddington outflows observed in GRS 1915+105, which imprint iron absorption features with equivalent widths of ~30 eV, the limits obtained here appear quite stringent, particularly when Holmberg IX X-1 and NGC 1313 X-1 must be expelling at least 5-10 times as much material if they host black holes of similar masses. The difficulty in reconciling these observational limits with the presence of strong line-of-sight outflows suggests that either these sources are not launching such outflows, or that they must be directed away from our viewing angle." @default.
• W3122889532 created "2021-02-01" @default.
• W3122889532 creator A5019923842 @default.
• W3122889532 creator A5024983697 @default.
• W3122889532 creator A5025039442 @default.
• W3122889532 creator A5043092604 @default.
• W3122889532 date "2012-09-18" @default.
• W3122889532 modified "2023-10-18" @default.
• W3122889532 title "Searching for massive outflows in Holmberg IX X-1 and NGC 1313 X-1: the iron<i>K</i>band" @default.
• W3122889532 cites W1480314585 @default.
• W3122889532 cites W1580022080 @default.
• W3122889532 cites W1757987097 @default.
• W3122889532 cites W1960085942 @default.
• W3122889532 cites W1983850825 @default.
• W3122889532 cites W1992067573 @default.
• W3122889532 cites W1999235136 @default.
• W3122889532 cites W2006844264 @default.
• W3122889532 cites W2015078230 @default.
• W3122889532 cites W2023080925 @default.
• W3122889532 cites W2030646506 @default.
• W3122889532 cites W2032117566 @default.
• W3122889532 cites W2053085244 @default.
• W3122889532 cites W2053488489 @default.
• W3122889532 cites W2055832107 @default.
• W3122889532 cites W2058609946 @default.
• W3122889532 cites W2060647152 @default.
• W3122889532 cites W2063592995 @default.
• W3122889532 cites W2068679152 @default.
• W3122889532 cites W2076129160 @default.
• W3122889532 cites W2078132064 @default.
• W3122889532 cites W2081785001 @default.
• W3122889532 cites W2084087407 @default.
• W3122889532 cites W2088819227 @default.
• W3122889532 cites W2101045281 @default.
• W3122889532 cites W2108584130 @default.
• W3122889532 cites W2108596190 @default.
• W3122889532 cites W2120915132 @default.
• W3122889532 cites W2124131920 @default.
• W3122889532 cites W2137096918 @default.
• W3122889532 cites W2141622247 @default.
• W3122889532 cites W2153543702 @default.
• W3122889532 cites W2154078330 @default.
• W3122889532 cites W2614392239 @default.
• W3122889532 cites W2950969827 @default.
• W3122889532 cites W3022917003 @default.
• W3122889532 cites W3027862860 @default.
• W3122889532 cites W3098284127 @default.
• W3122889532 cites W3098724979 @default.
• W3122889532 cites W3098912809 @default.
• W3122889532 cites W3099941437 @default.
• W3122889532 cites W3100071390 @default.
• W3122889532 cites W3100619045 @default.
• W3122889532 cites W3100671322 @default.
• W3122889532 cites W3101851556 @default.
• W3122889532 cites W3102773462 @default.
• W3122889532 cites W3102895663 @default.
• W3122889532 cites W3103038851 @default.
• W3122889532 cites W3103204359 @default.
• W3122889532 cites W3103385168 @default.
• W3122889532 cites W3103661837 @default.
• W3122889532 cites W3104500980 @default.
• W3122889532 cites W3106297564 @default.
• W3122889532 cites W3121174616 @default.
• W3122889532 cites W3123112321 @default.
• W3122889532 cites W3123307746 @default.
• W3122889532 cites W3123429667 @default.
• W3122889532 cites W3124695257 @default.
• W3122889532 cites W3125237935 @default.
• W3122889532 cites W4298876929 @default.
• W3122889532 doi "https://doi.org/10.1111/j.1365-2966.2012.21727.x" @default.
• W3122889532 hasPublicationYear "2012" @default.
• W3122889532 type Work @default.
• W3122889532 sameAs 3122889532 @default.
• W3122889532 citedByCount "26" @default.
• W3122889532 countsByYear W31228895322013 @default.
• W3122889532 countsByYear W31228895322014 @default.
• W3122889532 countsByYear W31228895322015 @default.
• W3122889532 countsByYear W31228895322016 @default.
• W3122889532 countsByYear W31228895322017 @default.
• W3122889532 countsByYear W31228895322020 @default.
• W3122889532 countsByYear W31228895322023 @default.
• W3122889532 crossrefType "journal-article" @default.
• W3122889532 hasAuthorship W3122889532A5019923842 @default.
• W3122889532 hasAuthorship W3122889532A5024983697 @default.
• W3122889532 hasAuthorship W3122889532A5025039442 @default.
• W3122889532 hasAuthorship W3122889532A5043092604 @default.
• W3122889532 hasBestOaLocation W31228895321 @default.
• W3122889532 hasConcept C120665830 @default.
• W3122889532 hasConcept C121332964 @default.
• W3122889532 hasConcept C125287762 @default.
• W3122889532 hasConcept C1276947 @default.
• W3122889532 hasConcept C198352243 @default.
• W3122889532 hasConcept C2524010 @default.
• W3122889532 hasConcept C2780928442 @default.
• W3122889532 hasConcept C33923547 @default.
• W3122889532 hasConcept C44870925 @default.
• W3122889532 hasConceptScore W3122889532C120665830 @default.
• W3122889532 hasConceptScore W3122889532C121332964 @default.

• next