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| Query : 2020RNAAS...4...98P |
2020RNAAS...4...98P - Research Notes of the AAS, 4, 98 (2020/June-0)
Origin of Sources of Repeating Fast Radio Bursts with Periodicity in Close Binary Systems.
POPOV S.B.
Abstract (from CDS):
It is proposed that sources of repeating fast radio bursts with detected periodicity are magnetars with extremely short initial spin periods at the protoneutron star stage, formed in binaries after tidal synchronization of their progenitor cores during late stages of thermonuclear burning in very close systems with orbital periods about a few days. This formation channel is in several respects different from evolution of progenitors of normal magnetars, and thus, it explains some differences between repeating and non-repeating sources of fast radio bursts.
Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.
Journal keyword(s): Neutron stars - Magnetars - Compact objects
Simbad objects: 2
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | FRB 20180916B | rB | 01 58 00.750 | +65 43 00.30 | ~ | 457 | 0 | |||||
| 2 | FRB 20181119D | rB | 05 31 58.6980 | +33 08 52.588 | ~ | 933 | 0 |
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