most citedAccretion Disk Spectra of the Brightest Ultra-luminous X-ray Source in M82

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astro-ph200857 cited

Optical Observations of SAX J1808.4-3658 During Quiescence

C. J. Deloye, C. O. Heinke, R. E. Taam +1

We observed the accreting millisecond pulsar SAX J1808.4-3658 with Gemini-South in g' and i' bands, nearly simultaneous with XMM-Newton observations. A clear periodic flux modulati…

astro-ph200836 cited

Common Envelope Mergers: A Possible Channel for Forming Single sdB Stars

Michael Politano, Ronald E. Taam, Marc van der Sluys +1

We quantify an evolutionary channel for single sdB stars based on mergers of binaries containing a red giant star and a lower mass main sequence or brown dwarf companion in our Gal…

astro-ph200858 cited

On the Properties of Inner Cool Disks in the Hard State of Black Hole X-Ray Transient Systems

Ronald E. Taam, B. F. Liu, F. Meyer +1

The formation of a cool disk in the innermost regions of black hole X-ray transient systems in the low hard state is investigated. Taking into account the combined cooling associat…

astro-ph200847 cited

The most massive progenitors of neutron stars: CXO J164710.2-455216

K. Belczynski, R. Taam

The evolution leading to the formation of a neutron star in the very young Westerlund 1 star cluster is investigated. The turnoff mass has been estimated to be 35 Msun, indicating…

astro-ph200788 cited

The Thermal Evolution of the Donors in AM CVn Binaries

Christopher J. Deloye, Ronald E. Taam, Christopher Winisdoerffer +1

(Abridged) We calculate the full stellar-structural evolution of donors in AM CVn systems formed through the WD channel coupled to the binary's evolution. Contrary to assumptions m…

astro-ph200637 cited

Accretion Disk Spectra of the Brightest Ultra-luminous X-ray Source in M82

Feng Yuan, Ronald E. Taam R. Misra, Xue-Bing Wu +1

Emission spectra of hot accretion disks characteristic of advection dominated accretion flow (ADAF) models are investigated for comparison with the brightest ultra-luminous source,…