Showing 1–20 of 29 results
/ Date/ Name
Sep 10, 2019The connection between merging double compact objects and the Ultraluminous X-ray SourcesJan 1, 2021High-redshift SMBHs can grow from stellar-mass seeds via chaotic accretionJan 7, 2003Accretion in Compact BinariesJan 16, 2006Short GRBs in old populations: Magnetars from WD-WD mergersAug 24, 2006The M-sigma Relation for Nucleated GalaxiesApr 15, 2007Progenitors of Long Gamma-ray BurstsSep 16, 2003Ultraluminous X-ray Sources and Star FormationApr 5, 2013BAL QSOs and Extreme UFOs: the Eddington connectionApr 16, 2011A relativistic jetted outburst from a massive black hole fed by a tidally disrupted starDec 18, 1999The Evolutionary Status of SS433Jan 4, 2012Clearing Out a GalaxyJan 31, 2015X-ray Transients: Hyper- or Hypo-Luminous?Nov 14, 2002A comparison of the acceleration mechanisms in YSO and AGN jetsDec 10, 2006An alternative to common envelope evolutionMar 15, 2012The observed $M - σ$ relations imply that SMBHs grow by cold chaotic accretionAug 7, 2012The M - σrelation in different environmentsAug 7, 2019Slow and fat: low-spin SMBHs are more massiveNov 18, 2016Radio pulse search and X-Ray monitoring of SAX J1808.4-3658: What Causes its Orbital Evolution?Apr 19, 2000The Population of Faint Transients in the Galactic CentreJul 5, 2000On a Theoretical Interpretation of the Period Gap in Binary Millisecond Pulsars