| 44 | | || '''03.05.2019[[BR]](11hrs, MPIA Hoersaal)''' || '''Anna Sippel''' || '''Black holes in globular clusters - A black hole love story'''[[BR]][[BR]]Globular clusters are some of the largest and heaviest star clusters and exist in and around galaxies, like our own Milky Way. Their stellar density is extremely high, inevitably leading to frequent encounters. At the same time, globular clusters house the final products of stellar evolution, such as black holes among others. In combination with the unique stellar dance in this very special environment at the center of a globular cluster, binary black holes can form. Using precise computer simulations I will show under which conditions these binary stars can eventually evolve to become gravitational wave sources. [[BR]][[BR]]Presentation: German[[BR]]Slides: German [[BR]]Questions: German, English || |
| | 44 | || '''03.05.2019[[BR]](11hrs, MPIA Hoersaal)''' || '''Anna Sippel''' || '''Black holes in globular clusters - A black hole love story'''[[BR]][[BR]]Globular clusters are some of the largest and heaviest star clusters and exist in and around galaxies, like our own Milky Way. Their stellar density is extremely high, inevitably leading to frequent encounters. At the same time, globular clusters house the final products of stellar evolution, such as black holes among others. In combination with the unique stellar dance in this very special environment at the center of a globular cluster, binary black holes can form. Using precise computer simulations I will show under which conditions these binary stars can eventually evolve to become gravitational wave sources. [[BR]][[BR]]Presentation: German[[BR]][https://svn.mpia.de/trac/gulli/att/raw-attachment/wiki/AlteVortraege2019S1/2019-05-03_BHLoveStory.pdf Slides: German] [[BR]]Questions: German, English || |
