ERRATUM: “SEARCH FOR CHAOS IN NEUTRON STAR SYSTEMS: IS Cyg X-3 A BLACK HOLE?” (2010, ApJ, 708, 862)

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

No Massive Black Hole in Cyg X-3

There has been a recent suggestion that Cyg X-3 contains a black hole (BH) of mass M1 ∼ 17M . This interpretation is closely linked to a previous claim that Cyg X-3 contains a Wolf-Rayet star of mass M2 ∼ 10M . The latter interpretation would imply that the X-ray source in this close binary (P = 4.8 hr) is enshrouded by a relatively cool superstrong wind with Ṁ ≥ 10 M yr. It can be shown that s...

متن کامل

Black hole-neutron star mergers for 10 M black holes

Francois Foucart, Matthew D. Duez, Lawrence E. Kidder, Mark A. Scheel, Bela Szilagyi, and Saul A. Teukolsky Center for Radiophysics and Space Research, Cornell University, Ithaca, New York, 14853, USA Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, Ontario M5S 3H8, Canada Department of Physics & Astronomy, Washington State University, Pullman, Washington 99164, ...

متن کامل

Coalescence of Black Hole-Neutron Star Binaries

We review the current status of general relativistic studies for the coalescence of black hole-neutron star (BH-NS) binaries. First, procedures for a solution of BH-NS binaries in quasi-equilibrium circular orbits and the numerical results, such as quasi-equilibrium sequence and mass-shedding limit, of the high-precision computation, are summarized. Then, the current status of numerical-relativ...

متن کامل

Prospects for gravitational-wave observations of neutron-star tidal disruption in neutron-star-black-hole binaries.

For an inspiraling neutron-star-black-hole (NS-BH) binary, we estimate the gravity-wave frequency f(td) at the onset of NS tidal disruption. We model the NS as a tidally distorted, homogeneous, Newtonian ellipsoid on a circular, equatorial geodesic around a Kerr BH. We find that f(td) depends strongly on the NS radius R, and estimate that LIGO-II (ca. 2006-2008) might measure R to 15% precision...

متن کامل

Cyg X - 3 : can the compact object be a black hole ?

By means of population synthesis we find that the expected Galactic number of black holes with massive helium star companions is ∼ 100 and depends on an assumed threshold for Mpre−BH. The overwhelming majority of these systems has orbital periods in excess of 10 hr, with a maximum at ∼ 100 hr, while under the Illarionov & Sunyaev(1975) disk formation criteria for accretion from the strong stell...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2010

ISSN: 0004-637X,1538-4357

DOI: 10.1088/0004-637x/715/1/697