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- W1671825388 abstract "System inclination angles have been determined for about 15 X-ray binaries, in which stellar mass black holes are considered to exist. These inclination angles range between 25 degrees and 80 degrees, but peaked between 60-70 degrees. This peak is not explained in the frame work of Newtonian gravity. However, this peak is reproduced naturally if we model the observed X-ray radiations as being produced in the accretion disks very close to the black hole horizons, where the extremely strong general and special relativistic effects, caused by the extremely strong gravity near the black hole horizons, modify the local radiation significantly as the X-rays propagate to the remote observer. Therefore the peak of the inclination angle distribution provides evidence or strong gravity around stellar mass black holes." @default.
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- W1671825388 date "2002-04-01" @default.
- W1671825388 modified "2023-09-27" @default.
- W1671825388 title "Inclination Angles of Black Hole X-Ray Binaries Manifest Strong Gravity around Black Holes" @default.
- W1671825388 hasPublicationYear "2002" @default.
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