Matches in SemOpenAlex for { <https://semopenalex.org/work/W1989587060> ?p ?o ?g. }
- W1989587060 endingPage "2515" @default.
- W1989587060 startingPage "2500" @default.
- W1989587060 abstract "The existing radio and X-ray flux correlation for Galactic black holes in the hard and quiescent states relies on a sample which is mostly dominated by two sources (GX 339-4 and V404 Cyg) observed in a single outburst. In this paper, we report on a series of radio and X-ray observations of the recurrent black hole GX 339-4 with the Australia Telescope Compact Array, the Rossi X-ray Timing Explorer and the Swift satellites. With our new long term campaign, we now have a total of 88 quasi-simultaneous radio and X-ray observations of GX 339-4 during its hard state, covering a total of seven outbursts over a 15--year period. Our new measurements represent the largest sample for a stellar mass black hole, without any bias from distance uncertainties, over the largest flux variations and down to a level that could be close to quiescence, making GX 339-4 the reference source for comparison with other accreting sources (black holes, neutrons stars, white dwarfs and active galactic nuclei). Our results demonstrate a very strong and stable coupling between radio and X-ray emission, despite several outbursts of different nature and separated by a period of quiescence. The radio and X-ray luminosity correlation of the form L_X ~L_Rad^0.62 +/-0.01 confirms the non-linear coupling between the jet and the inner accretion flow powers and better defines the standard correlation track in the radio-X-ray diagram for stellar mass black holes. We further note epochs of deviations from the fit that significantly exceed the measurement uncertainties, especially during the formation and destruction of the compact jets ...[abridged]. We incorporated our new data in a more global study of black hole candidates strongly supporting a scale invariance in the jet-accretion coupling of accreting black holes, and confirms the existence of two populations of sources in the radio/X-ray diagram." @default.
- W1989587060 created "2016-06-24" @default.
- W1989587060 creator A5004465093 @default.
- W1989587060 creator A5004495261 @default.
- W1989587060 creator A5018034654 @default.
- W1989587060 creator A5020511005 @default.
- W1989587060 creator A5042161585 @default.
- W1989587060 creator A5047121906 @default.
- W1989587060 creator A5068028807 @default.
- W1989587060 creator A5086737368 @default.
- W1989587060 date "2012-11-28" @default.
- W1989587060 modified "2023-10-15" @default.
- W1989587060 title "The ‘universal’ radio/X-ray flux correlation: the case study of the black hole GX 339−4" @default.
- W1989587060 cites W1783818038 @default.
- W1989587060 cites W1798864014 @default.
- W1989587060 cites W1903446574 @default.
- W1989587060 cites W1964974519 @default.
- W1989587060 cites W1965997551 @default.
- W1989587060 cites W1968514632 @default.
- W1989587060 cites W1970417976 @default.
- W1989587060 cites W1976409167 @default.
- W1989587060 cites W1977984384 @default.
- W1989587060 cites W1978701186 @default.
- W1989587060 cites W1978745084 @default.
- W1989587060 cites W1987913674 @default.
- W1989587060 cites W1997370179 @default.
- W1989587060 cites W2002993223 @default.
- W1989587060 cites W2005965717 @default.
- W1989587060 cites W2007036736 @default.
- W1989587060 cites W2009154954 @default.
- W1989587060 cites W2011042489 @default.
- W1989587060 cites W2019189995 @default.
- W1989587060 cites W2023721823 @default.
- W1989587060 cites W2035906567 @default.
- W1989587060 cites W2039866073 @default.
- W1989587060 cites W2040407016 @default.
- W1989587060 cites W2044094489 @default.
- W1989587060 cites W2048206598 @default.
- W1989587060 cites W2050276909 @default.
- W1989587060 cites W2050891937 @default.
- W1989587060 cites W2052172883 @default.
- W1989587060 cites W2052730169 @default.
- W1989587060 cites W2056376181 @default.
- W1989587060 cites W2056985806 @default.
- W1989587060 cites W2058387383 @default.
- W1989587060 cites W2066893209 @default.
- W1989587060 cites W2072670786 @default.
- W1989587060 cites W2081820201 @default.
- W1989587060 cites W2081851528 @default.
- W1989587060 cites W2086423889 @default.
- W1989587060 cites W2087885535 @default.
- W1989587060 cites W2095030862 @default.
- W1989587060 cites W2096164418 @default.
- W1989587060 cites W2101769690 @default.
- W1989587060 cites W2107051429 @default.
- W1989587060 cites W2107359327 @default.
- W1989587060 cites W2107543427 @default.
- W1989587060 cites W2109467954 @default.
- W1989587060 cites W2110317800 @default.
- W1989587060 cites W2111434714 @default.
- W1989587060 cites W2112261839 @default.
- W1989587060 cites W2113978543 @default.
- W1989587060 cites W2113986346 @default.
- W1989587060 cites W2115949825 @default.
- W1989587060 cites W2117710713 @default.
- W1989587060 cites W2122342311 @default.
- W1989587060 cites W2126149981 @default.
- W1989587060 cites W2130507340 @default.
- W1989587060 cites W2130592261 @default.
- W1989587060 cites W2131123502 @default.
- W1989587060 cites W2131839509 @default.
- W1989587060 cites W2148110644 @default.
- W1989587060 cites W2148115088 @default.
- W1989587060 cites W2149532224 @default.
- W1989587060 cites W2151513600 @default.
- W1989587060 cites W2953105268 @default.
- W1989587060 cites W2989887117 @default.
- W1989587060 cites W3028849884 @default.
- W1989587060 cites W3098292104 @default.
- W1989587060 cites W3098410660 @default.
- W1989587060 cites W3098477867 @default.
- W1989587060 cites W3098535039 @default.
- W1989587060 cites W3098610057 @default.
- W1989587060 cites W3098841953 @default.
- W1989587060 cites W3099049655 @default.
- W1989587060 cites W3099240080 @default.
- W1989587060 cites W3099401213 @default.
- W1989587060 cites W3099410783 @default.
- W1989587060 cites W3099745664 @default.
- W1989587060 cites W3099875197 @default.
- W1989587060 cites W3100947325 @default.
- W1989587060 cites W3100949598 @default.
- W1989587060 cites W3101413436 @default.
- W1989587060 cites W3101655862 @default.
- W1989587060 cites W3102043407 @default.
- W1989587060 cites W3102360080 @default.
- W1989587060 cites W3102369283 @default.
- W1989587060 cites W3103861105 @default.