Nulling Phenomenon of the New Radio Pulsar J0810+37 at a Frequency of 111 MHz


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

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.

作者简介

D. Teplykh

Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute

Email: malofeev@prao.ru
俄罗斯联邦, 1A Radioteleskopnaya St., Pushchino, Moscow oblast, 142290

V. Malofeev

Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute

编辑信件的主要联系方式.
Email: malofeev@prao.ru
俄罗斯联邦, 1A Radioteleskopnaya St., Pushchino, Moscow oblast, 142290

补充文件

附件文件
动作
1. JATS XML

版权所有 © Allerton Press, Inc., 2019