Black Holes
Recent progress in black hole research is illustrated by three examples. We discuss the observational challenges that were met to show that a supermassive black hole exists at the center of our galaxy. Stellar-size black holes have been studied in x-ray binaries and microquasars. Finally, numerical...
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| Veröffentlicht in: | Proceedings of the National Academy of Sciences - PNAS 2001-09, Vol.98 (19), p.10525-10526 |
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| container_issue | 19 |
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| container_title | Proceedings of the National Academy of Sciences - PNAS |
| container_volume | 98 |
| creator | Brügmann, B. Ghez, A.M. Greiner, J. |
| description | Recent progress in black hole research is illustrated by three examples. We discuss the observational challenges that were met to show that a supermassive black hole exists at the center of our galaxy. Stellar-size black holes have been studied in x-ray binaries and microquasars. Finally, numerical simulations have become possible for the merger of black hole binaries. |
| doi_str_mv | 10.1073/pnas.201365798 |
| format | Article |
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| identifier | ISSN: 0027-8424 |
| ispartof | Proceedings of the National Academy of Sciences - PNAS, 2001-09, Vol.98 (19), p.10525-10526 |
| issn | 0027-8424 1091-6490 |
| language | eng |
| recordid | cdi_pubmedcentral_primary_oai_pubmedcentral_nih_gov_58496 |
| source | JSTOR Archive Collection A-Z Listing; PubMed Central; Alma/SFX Local Collection; Free Full-Text Journals in Chemistry |
| subjects | Accretion disks Adaptive optics Binary stars Binary system Black holes From the Academy From the Academy: German-American Frontiers of Science Symposium Milky Way Galaxy Physics Solar mass Stars Stars & galaxies Supermassive black holes X ray binary stars |
| title | Black Holes |
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