Very Low Frequency QPO in 4U1700-37

Abstract

Very low frequency (ν ~ 1.9 mHz) quasi-periodic oscillations (QPO) have been detected in 2 - 60 keV X-rays from 4U1700-37 using auto-correlation function analysis of RXTE archival data. No pulsar signal was detected in the data. Less than 0.5% of the flux from the source (3σ upper limit) is coherently pulsed with a period between 250 ms and 40 s. This upper limit corresponds to a pulsed flux <0.02 mJy. The existence of QPO in 4U1700-37 and the lack of a detected pulsar indicates that the X-ray source is more likely to be a black hole than a neutron star, consistent with recent mass estimates.

Cited by in corpus (2)

• Spectroscopic evidence for a low-mass black hole in SWIFT J1753.5-0127
• Evidence of Compton cooling during an X-ray flare supports a neutron star nature of the compact object in 4U1700-37