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Another paper on GW170817
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Send message Joined: 25 Feb 15 Posts: 50 Credit: 5,684,705 RAC: 0 |
Sorry for late notification! Another research on the famous GW170817 source, which used data obtained from the Universe@Home project, have been published last year. In this study, it was shown that the merger rates of double neutron stars (calculated from one direct observation) stay in contradiction with these inferred from the observations of double pulsars in our Galaxy. The reason behind this tension is the delay time distribution which favours short delays. The study highlights the problem that scientist encounter trying to connect evolutionary predictions and the observations of the first double neutron star merger. The original paper can be found here: http://adsabs.harvard.edu/abs/2018arXiv181210065B Grzegorz Wiktorowicz National Astronomical Observatories, Chinese Academy of Sciences |
Send message Joined: 6 Feb 19 Posts: 41 Credit: 131,325,319 RAC: 0 |
Awesome |
Send message Joined: 8 May 19 Posts: 1 Credit: 0 RAC: 0 |
Hi every one |