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astro-ph1999★ 27 cited
Constraints on the Steady-State R-mode Amplitude in Neutron Star Transients
Edward F. Brown, Greg Ushomirsky
Recent observations suggest that neutron stars in low-mass X-ray binaries rotate within a narrow range of spin frequencies clustered around 300 Hz. A proposed explanation for this…
astro-ph1999★ 81 cited
A Method for Distinguishing Between Transiently Accreting Neutron Stars and Black Holes, in Quiescence
Robert E. Rutledge, Lars Bildsten, Edward F. Brown +2
We fit hydrogen atmosphere models to the X-ray data for four neutron stars (three from a previous paper, plus 4U 2129+47) and six black hole candidates (A0620-00, GS 2000+25, GS 11…