A NEW DYNAMICAL MODEL FOR THE BLACK HOLE BINARY LMC X-1

A NEW DYNAMICAL MODEL FOR THE BLACK HOLE BINARY LMC X-1

We present a dynamical model of the high mass X-ray binary LMC X-1 based on high-resolution optical spectroscopy and extensive optical and near-infrared photometry. From our new optical data we find an orbital period of P = 3.90917 ± 0.00005 days. We present a refined analysis of the All Sky Monitor...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής
Κύριοι συγγραφείς: Orosz, Jerome A., Steeghs, Danny, McClintock, Jeffrey E., Torres, Manuel A. P., Bochkov, Ivan, Gou, Lijun, Narayan, Ramesh, Blaschak, Michael, Bailyn, Charles D., Dwyer, Morgan, Buxton, Michelle, Levine, Alan M, Remillard, Ronald A
Άλλοι συγγραφείς: MIT Kavli Institute for Astrophysics and Space Research
Μορφή: Άρθρο
Γλώσσα:en_US
Έκδοση: Institute of Physics/American Astronomical Society 2015
Διαθέσιμο Online:http://hdl.handle.net/1721.1/96090

Διαδίκτυο

http://hdl.handle.net/1721.1/96090

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