1999/04/28 by Eric C. Ford · 1 citation
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysical Phenomena and Observations #Earth Systems and Cosmic Evolution #Gamma-ray bursts and supernovae #astro-ph
paper · pdf · doi:10.1086/312108
accepted ApJ Letters
arxiv created 1999/04/28 · openalex publication_date 1999/07/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/04
Numerous X-ray bursts show strong oscillations in their flux at several hundred hertz as revealed by Rossi X-Ray Timing Explorer . Analyzing one such oscillation from the X-ray binary Aquila X-1, I find that low-energy photons (3.5-5.7 keV) lag high-energy photons (>5.7 keV) by approximately 1 rad. The oscillations are thought to be produced by hot spots on the spinning neutron star. The lags can then be explained by a Doppler shifting of emission from the hot spots, higher-energy photons being emitted earlier in the spin phase as the spot approaches the observer. A quantitative test of this simple model shows a remarkable agreement with the data. Similar low-energy lags have been measured in kilohertz quasi-periodic oscillations and in the accreting millisecond pulsar SAX J1808.4-3658. A Doppler delay mechanism may be at work there as well.