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- Publications
- Influence
Thermonuclear (Type I) X-Ray Bursts Observed by the Rossi X-Ray Timing Explorer
- D. Galloway, M. Muno, J. Hartman, D. Psaltis, D. Chakrabarty
- Physics
- 11 August 2006
We have assembled a sample of 1187 thermonuclear (type I) X-ray bursts from observations of 48 accreting neutron stars by the Rossi X-ray Timing Explorer, spanning more than 10 years. The sample… Expand
Neutron Star Mass Measurements. I. Radio Pulsars
- S. Thorsett, D. Chakrabarty
- Physics
- 22 March 1998
There are now about 50 known radio pulsars in binary systems, including at least five in double neutron star binaries. In some cases, the stellar masses can be directly determined from measurements… Expand
Observations of Accreting Pulsars
- L. Bildsten, D. Chakrabarty, +10 authors R. Wilson
- Physics
- 10 July 1997
We discuss recent observations of accreting binary pulsars with the all-sky BATSE instrument on the Compton Gamma Ray Observatory. BATSE has detected and studied nearly half of the known accreting… Expand
An ultraluminous X-ray source powered by an accreting neutron star
- M. Bachetti, F. Harrison, +21 authors W. Zhang
- Physics, Medicine
- Nature
- 9 October 2014
The majority of ultraluminous X-ray sources are point sources that are spatially offset from the nuclei of nearby galaxies and whose X-ray luminosities exceed the theoretical maximum for spherical… Expand
The two-hour orbit of a binary millisecond X-ray pulsar
- D. Chakrabarty, E. Morgan
- Physics
- Nature
- 23 April 1998
Typical radio pulsars are magnetized neutron stars that are born rapidly rotating and slow down as they age on time scales of 10 to 100 million years. In contrast, millisecond radio pulsars spin very… Expand
A debris disk around an isolated young neutron star
- Z. Wang, D. Chakrabarty, D. Kaplan
- Physics, Medicine
- Nature
- 4 April 2006
Pulsars are rotating, magnetized neutron stars that are born in supernova explosions following the collapse of the cores of massive stars. If some of the explosion ejecta fails to escape, it may fall… Expand
Discovery of a High-Latitude Accreting Millisecond Pulsar in an Ultracompact Binary
- D. Galloway, D. Chakrabarty, E. Morgan, R. Remillard
- Physics
- 27 June 2002
We have identified the third known accretion-powered millisecond pulsar, XTE J0929-314, with the Rossi X-Ray Timing Explorer. The source is a faint, high Galactic latitude X-ray transient (d 5 kpc)… Expand
The Disk-Magnetosphere Interaction in the Accretion-powered Millisecond Pulsar SAX J1808.4–3658
- D. Psaltis, D. Chakrabarty
- Physics
- 25 September 1998
The recent discovery of the first known accretion-powered millisecond pulsar with the Rossi X-Ray Timing Explorer provides the first direct probe of the interaction of an accretion disk with the… Expand
Rapid Spin-Up Episodes in the Wind-fed Accreting Pulsar GX 301–2
- Danny T. Koh, L. Bildsten, +9 authors B. Rubin
- Physics
- 20 April 1997
The accreting pulsar GX 301-2 (P = 680 s) has been observed continuously by the large-area detectors of the Burst and Transient Source Experiment (BATSE) instrument on the Compton Gamma Ray… Expand
The Long-Term Evolution of the Spin, Pulse Shape, and Orbit of the Accretion-powered Millisecond Pulsar SAX J1808.4–3658
- J. Hartman, A. Patruno, +10 authors Naval Research Lab
- Physics
- 1 August 2007
We present a 7 yr timing study of the 2.5 ms X-ray pulsar SAX J1808.4–3658, an X-ray transient with a recurrence time of 2 yr, using data from the Rossi X-Ray Timing Explorer covering four transient… Expand
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