PofoliaShared via Pofolia

Science· 2013Q1

A Massive Pulsar in a Compact Relativistic Binary

John Antoniadis, P. C. C. Freire, Norbert Wex, Thomas M. Tauris et al.

Short summary

A 2.01 solar mass pulsar in a 2.46-hour orbit with a white dwarf provides the first test of general relativity in a strong-field regime, with observed orbital decay matching GR predictions.

AI-generated from the title and abstract; the full text is not read.

TakeawaysIn the app
Key pointsIn the app
Ask the paperIn the app

The rest is in the Pofolia app

Takeaways, key points and questions to the paper; new summaries every day for your field. Free.

Sign in on the web to open

Field: Astronomy and Astrophysics

Astronomy and AstrophysicsPhysics and Astronomy