

"Race tracks" followed by a pair of two unequal mass black holes with misaligned spins. The orbits are precessing. The two black holes have formed a common horizon, which is shown as a third surface around the two individucal horizons. (SXS Collaboration, learn more)
"Race tracks" followed by a pair of two unequal mass black holes with misaligned spins. The orbits are precessing. The two black holes have formed a common horizon, which is shown as a third surface around the two individucal horizons. (SXS Collaboration, learn more)
比特安卓版下载 is part of the Division of Physics, Mathematics, and Astronomy at Caltech. We are located in the Cahill Center for Astronomy and Astrophysics.
Next TAPIR Seminar is Fri, March 13, Robert Fisher, UMass Dartmouth, Type Ia Supernovae Progenitors Zoom: http://caltech.zoom.us/j/121393738
Meeting ID: 121 393 738