Abstract
The eclipses of certain types of binary millisecond pulsars (i.e. 'black widows' and 'redbacks') are often studied using high-time-resolution, 'beamformed' radio observations. However, they may also be detected in images generated from interferometric data. As part of a larger imaging project to characterize the variable and transient sky at radio frequencies -0.4), such that the pulsar is eclipsed for longer at lower frequencies, in broad agreement with beamformed studies of other similar sources. Furthermore, the detection of the eclipses in imaging data suggests an eclipsing medium that absorbs the pulsed emission, rather than scattering it. Our study is also a demonstration of the prospects of finding pulsars in wide-field imaging surveys with the current generation of low-frequency radio telescopes.
Original language | English |
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Pages (from-to) | 2681-2689 |
Number of pages | 9 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 459 |
Issue number | 3 |
Early online date | 8 Apr 2016 |
DOIs | |
Publication status | Published - 1 Jul 2016 |
Keywords
- Binaries: eclipsing
- Pulsars: general
- Pulsars: individual: PSR J2215+5135
- Radio continuum: stars