A RetroSearch Logo

Home - News ( United States | United Kingdom | Italy | Germany ) - Football scores

Search Query:

Showing content from https://link.springer.com/article/10.12942/lrr-2014-3/figures/3 below:

Figure 3 | The Evolution of Compact Binary Star Systems

The maximum initial orbital period (in hours) of two point masses that will coalesce due to gravitational wave emission in a time interval shorter than 1010 yr, as a function of the initial eccentricity e0. The lines are calculated for 10 M + 10 M (BH + BH), 10 M + 1.4 M (BH + NS), and 1.4 M +1.4 M (NS + NS).

Back to article page

RetroSearch is an open source project built by @garambo | Open a GitHub Issue

Search and Browse the WWW like it's 1997 | Search results from DuckDuckGo

HTML: 3.2 | Encoding: UTF-8 | Version: 0.7.4