Mass of black holes: The State of the Art Export

@article{citeulike:5897629, abstract = {In this small review we present the actual state the knowledge about weighting black holes. Black holes can be found in stellar binary systems in our Galaxy and in other nearby galaxies, in globular clusters, which we can see in our and nearby galaxies, and in centres of all well-developed galaxies. Range of values of their masses is wide and cover about ten orders of magnitude (not taking into account the hypothetic primordial black holes). Establishing the presence of black holes, and in particular the measurement of their mass is one on the key issues for many branches of astronomy, from stellar evolution to cosmology.}, archivePrefix = {arXiv}, author = {Czerny, B. and Nikolajuk, M.}, citeulike-article-id = {5897629}, citeulike-linkout-0 = {http://arxiv.org/abs/0910.0313}, citeulike-linkout-1 = {http://arxiv.org/pdf/0910.0313}, day = {2}, eprint = {0910.0313}, keywords = {bhs}, month = {Oct}, posted-at = {2009-10-06 10:19:31}, priority = {2}, title = {Mass of black holes: The State of the Art}, url = {http://arxiv.org/abs/0910.0313}, year = {2009} }

TY - JOUR ID - citeulike:5897629 L3 - citeulike-article-id:5897629 N2 - In this small review we present the actual state the knowledge about weighting black holes. Black holes can be found in stellar binary systems in our Galaxy and in other nearby galaxies, in globular clusters, which we can see in our and nearby galaxies, and in centres of all well-developed galaxies. Range of values of their masses is wide and cover about ten orders of magnitude (not taking into account the hypothetic primordial black holes). Establishing the presence of black holes, and in particular the measurement of their mass is one on the key issues for many branches of astronomy, from stellar evolution to cosmology. TI - Mass of black holes: The State of the Art KW - bhs AU - Czerny, B AU - Nikolajuk, M PY - 2009/Oct/02/ UR - http://arxiv.org/abs/0910.0313 ER -