Scenarios for GCRT J1745-3009

2008/12/25 by С. Б. Попов, S. B. Popov, Popov, S. B. · 2 citations
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Geophysics and Gravity Measurements #Pulsars and Gravitational Waves Research #astro-ph

paper · pdf · doi:10.48550/arxiv.0812.4587

8 pages, no figures, Talk at the conference "VA100 Evolution of Cosmic Objects Through Their Physical Activity", Yerevan, Armenia 2008. Subm. to the proceedings

arxiv created 2008/12/25 · openalex publication_date 2008/12/25 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

I discuss several scenarios to explain properties of the radio transient source GCRT J1745-3009. Namely, a highly magnetized neutron star on the propeller or georotator stage, a transient propeller, and an ejector in a binary system are discussed. Simple populational estimates favor the transient propeller model.

Cited by

• Low-frequency observations of low-mass binary systems with neutron star candidates
• Are the distributions of fast radio burst properties consistent with a cosmological population?

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