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10.1038/ncomms14906 http://scihub22266oqcxt.onion/10.1038/ncomms14906 C5382320!5382320!28378739     free     free     free Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       Nat+Commun 2017 ; 8 (ä): ä Nephropedia Template TP {{tp|p=28378739|t=2017. Formation of the first three gravitational-wave observations through isolated binary evolution |pdf=|usr=}}{{28378739}} gab.com Text Formation of the first three gravitational-wave observations through isolated binary evolution JO: Nat Commun http://www.kidney.de/pget.php?&tw=1&pmid=28378739 #FOAvip During its first four months of taking data, Advanced LIGO has detected gravitational waves from two binary black hole mergers, GW150914 and GW151226, along with the statistically less significant binary black hole merger candidate LVT151012. Here we use the rapid binary population synthesis code COMPAS to show that all three events can be explained by a single evolutionary channel?classical isolated binary evolution via mass transfer including a common envelope phase. We show all three events could have formed in low-metallicity environments (Z=0.001) from progenitor binaries with typical total masses ?160M?, ?60M? and ?90M?, for GW150914, GW151226 and LVT151012, respectively. Twit Text FOAVip Formation of the first three gravitational-wave observations through isolated binary evolution ????Nat Commun http://www.kidney.de/pget.php?&tw=1&pmid=28378739 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=28378739 #FOAvip English Wikipedia <ref>{{Cite pmid|28378739}}</ref> Formation of the first three gravitational-wave observations through isolated binary evolution #MMPMID28378739 Stevenson S; Vigna-Gómez A; Mandel I; Barrett JW; Neijssel CJ; Perkins D; de Mink SE Nat Commun 2017[]; 8 (ä): ä PMID28378739show ga During its first four months of taking data, Advanced LIGO has detected gravitational waves from two binary black hole mergers, GW150914 and GW151226, along with the statistically less significant binary black hole merger candidate LVT151012. Here we use the rapid binary population synthesis code COMPAS to show that all three events can be explained by a single evolutionary channel?classical isolated binary evolution via mass transfer including a common envelope phase. We show all three events could have formed in low-metallicity environments (Z=0.001) from progenitor binaries with typical total masses ?160M?, ?60M? and ?90M?, for GW150914, GW151226 and LVT151012, respectively. äFormation of the first three gravitational-wave observations through i(epmc).pdf DeepDyve Pubget Overpricing