Discovering stellar core collapse events using satellite-born RF detectors

Details Discovering stellar core collapse events using satellite-born RF detectors Discovering stellar core collapse events using satellite-born RF detectors

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap%26ss.314..275m&link_type=abstract

Astrophysics and Space Science, Volume 314, Issue 4, pp.275-279

Astronomy and Astrophysics

Astrophysics

Radiation Mechanism: General

Scientific paper

Previous research has shown that a massive electromagnetic pulse (MEMP) is the precursor to type II stellar core collapse events. While Earth’s ionosphere makes ground-based detection of this RF (radio frequency) electromagnetic pulse improbable, it can be readily observed by satellite-born detectors. The expected radius of detection using presently available COTS (commercial-off-the-shelf) equipment is 2.67 billion light-years. A new class of astronomical objects is predicted to exist.

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