Nulling Phenomenon of the New Radio Pulsar J0810+37 at a Frequency of 111 MHz
- Authors: Teplykh D.A.1, Malofeev V.M.1
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Affiliations:
- Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
- Issue: Vol 46, No 12 (2019)
- Pages: 380-382
- Section: Article
- URL: https://journal-vniispk.ru/1068-3356/article/view/229126
- DOI: https://doi.org/10.3103/S1068335619120030
- ID: 229126
Cite item
Abstract
Pulsar J0810+37 with a period of 1.2483 s is detected at a frequency of 111 MHz during the pulsar search at the Big Scanning Antenna (BSA) radio telescope of the Lebedev Physical Institute [1]. In this paper, we present the results of the detailed study of radio emission from J0810+37 which exhibits a rare nulling effect of different durations in a very wide time interval with an average nulling fraction in “switch-on” days 〈NF〉 = 38%; considering “switch-off” days, 〈NF〉 = 74%, since radio emission from this source is interrupted on average by 2–3 days, and then it again revives on average for 1–2 days. The “switch-off” periods reach 7 days.
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About the authors
D. A. Teplykh
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
Email: malofeev@prao.ru
Russian Federation, 1A Radioteleskopnaya St., Pushchino, Moscow oblast, 142290
V. M. Malofeev
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
Author for correspondence.
Email: malofeev@prao.ru
Russian Federation, 1A Radioteleskopnaya St., Pushchino, Moscow oblast, 142290
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