2021/03/08 by Н. Н. Чугай, Chugai, N. N., A. D. Kudryashov +1
Physics and Astronomy · #Astrophysical Phenomena and Observations #Atomic and Molecular Physics #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #X-ray Spectroscopy and Fluorescence Analysis
paper · pdf · doi:10.48550/arxiv.2103.04716
openalex publication_date 2021/03/08 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We explore for the first time effects of the magnetic field on the escape of 22Na positrons and on the flux evolution of annihilation 511 keV line in novae. It is shown that for the white dwarf magnetic field of ∼ 106 G the field of the expanding nova shell is able to significantly impede positrons escape and increase the time of the nova emission in 511keV up to hundreds days.