Discovery of a 69 Millisecond X-Ray Pulsar: A Compact Source in the Vicinityof the Supernova Remnant RCW 103 [PDF]
, 1998 K. Torii +8 more
openalex +1 more source
Stellar forensics - II. Millisecond pulsar binaries [PDF]
, 1998 Brad M. S. Hansen, E. S. Phinney
openalex +1 more source
Repeating fast radio burst 20201124A originates from a magnetar/Be star binary. [PDF]
Nat Commun, 2022 Wang FY, Zhang GQ, Dai ZG, Cheng KS.
europepmc +1 more source
Millisecond and binary pulsars as nature's frequency standards -- I. A generalized statistical model of low-frequency timing noise [PDF]
, 1997 Sergei M. Kopeikin
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Recovering Pulsar Braking Index from a Population of Millisecond Pulsars
The Astrophysical JournalThe braking index, n , of a pulsar is a measure of its angular momentum loss and the value it takes to correspond to different spin-down mechanisms. For a pulsar spinning down due to gravitational-wave emission from the principal mass quadrupole mode ...
A. L. Hewitt, M. Pitkin, I. M. Hook
doaj +1 more source
A commentary of "Consistency radio bursts in the Milky Way": 10 remarkable discoveries from 2020 in Nature. [PDF]
Fundam Res, 2022 Li D.
europepmc +1 more source
Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]
Nat Astron, 2022 Caleb M +21 more
europepmc +1 more source
The Temperature and Cooling Age of the White Dwarf Companion to the Millisecond Pulsar PSR B1855+09 [PDF]
, 2000 M. H. van Kerkwijk +3 more
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Comparison of giant radio pulses in young pulsars and millisecond pulsars
, 2007 Pulse-to-pulse intensity variations are a common property of pulsar radio emission. For some of the objects single pulses are often 10-times stronger than their average pulse. The most dramatic events are so-called giant radio pulses (GRPs).
Jessner, A. +3 more
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