X-ray spectroscopy of the ADC source X1822-371 with Chandra and XMM-Newton
Context. The eclipsing low-mass X-ray binary X1822-371 is the prototype of the accretion
disc corona (ADC) sources. Its inclination angle (≃ 82.5°) is high enough that flux from the …
disc corona (ADC) sources. Its inclination angle (≃ 82.5°) is high enough that flux from the …
Tomography of X-ray Nova Muscae 1991: evidence for ongoing mass transfer and stream–disc overflow
We present a spectroscopic analysis of the black hole binary Nova Muscae 1991 in
quiescence using data obtained in 2009 with Magellan Echelette on the Magellan Clay …
quiescence using data obtained in 2009 with Magellan Echelette on the Magellan Clay …
Phase-resolved spectroscopy of the low-mass X-ray binary V801 Ara
We present phase-resolved optical spectra of the low-mass X-ray binary system V801 Ara.
The spectra, obtained in 2014 with Inamori Magellan Areal Camera and Spectrograph on …
The spectra, obtained in 2014 with Inamori Magellan Areal Camera and Spectrograph on …
[PDF][PDF] Precision ephemerides of neutron-star binaries to assist gravitational-wave searches: Sco X-1 & Cyg X-2
SS Premachandra - 2015 - scholar.archive.org
Sco X-1 was the first extrasolar X-ray source discovered, in 1962 with an Aerobee rocket
instrumented with Geiger counters (Giacconi et al., 1962). It is the brightest persistent X-ray …
instrumented with Geiger counters (Giacconi et al., 1962). It is the brightest persistent X-ray …