电邮这篇文章 Detection of radio emission from magnetar RX J1605.3+3249 at frequency 111 MHz
- 作者: Rodin A.E.1, Fedorova V.A.1
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隶属关系:
- P. N. Lebedev Physical Institute of the Russian Academy of Sciences
- 期: 卷 102, 编号 6 (2025)
- 页面: 490-495
- 栏目: Articles
- URL: https://bakhtiniada.ru/0004-6299/article/view/308342
- DOI: https://doi.org/10.31857/S0004629925060048
- EDN: https://elibrary.ru/qawhmy
- ID: 308342
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详细
For the first time, pulsed radio emission from the magnetar RX J1605.3+3249, which is part of the “magnificent seven”, has been detected. Data obtained at the BSA LPI radio telescope at a frequency of 111 MHz in the period from 2012 to 2024 were processed. The peak flux density mJy and the dispersion measure pc/cm3 were measured.
作者简介
A. Rodin
P. N. Lebedev Physical Institute of the Russian Academy of Sciences
Email: a.rodin@lebedev.ru
Moscow, Russia
V. Fedorova
P. N. Lebedev Physical Institute of the Russian Academy of Sciences
Email: v.fedorova@lebedev.ru
Moscow, Russia
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