REVIEW 1 cited by
BeppoSAX Observations of the Atoll X-Ray Binary 4U0614+091
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
We report the first simultaneous measurement of the broad band X-ray (0.3-150 keV) spectrum of the neutron star x-ray binary 4U0614+091. Our data confirm the presence of a hard x-ray tail that can be modeled as thermal Comptonization of low-energy photons on electrons having a very high temperature, greater than 220 keV, or as a non-thermal powerlaw. We detected a spectral feature that can be interpreted as reprocessing, via Compton reflection, of the direct emission by an optically-thick disk and found a correlation between the photon index of the power-law tail and the fraction of radiation reflected which is similar to the correlation found for black hole candidate x-ray binaries and Seyfert galaxies.
Forward citations
Cited by 1 Pith paper
-
Continuous gravitational waves from thermal mountains on accreting neutron stars: effect of the nuclear pasta phase
Including the nuclear pasta layer raises the predicted continuous gravitational-wave quadrupole moment of accreting neutron stars to about 1.7e39 g cm^2, making known sources detectable by next-generation ground-based...
Discussion (0). Continue with ORCID to comment.