The low-spin black hole in LMC X-3

Building upon a new dynamical model for the X-ray binary LMC X-3, we measure the spin of its black hole (BH) primary via the continuum-fitting method. We consider over one thousand thermal-state Rossi X-ray Timing Explorer X-ray spectra of LMC X-3. Using a large subset of these spectra, we constrain...

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Bibliografski detalji
Glavni autori: Steiner, James F., McClintock, Jeffrey E., Orosz, Jerome A., Bailyn, Charles D., Kolehmainen, Mari, Straub, Odele, Remillard, Ronald A
Daljnji autori: MIT Kavli Institute for Astrophysics and Space Research
Format: Članak
Jezik:en_US
Izdano: IOP Publishing 2015
Online pristup:http://hdl.handle.net/1721.1/92991