Peculiarities of radio emission from new pulsars at 111 MHz
- Authors
- Type
- Published Article
- Journal
- Open Astronomy
- Publisher
- De Gruyter
- Publication Date
- Apr 18, 2022
- Volume
- 31
- Issue
- 1
- Pages
- 166–171
- Identifiers
- DOI: 10.1515/astro-2022-0019
- Source
- De Gruyter
- Keywords
- Disciplines
- License
- Green
Abstract
The analysis of radio emission of three new pulsars discovered at the Pushchino Radio Astronomy Observatory is presented. The detailed observations were carried out at a frequency of 111 MHz using the large phase array and the standard digital receiver with a total bandwidth of 2.245 MHz and a time resolution of 2.46 or 5.12 ms. All pulsars exhibit features of their radiation, the subpulse drift is observed in J0220+3622, the flare activity is exhibited in J0303+2248, and the nulling phenomenon has been detected in J0810+3725.
