Work

Detection of Radio Emissions from Magnetar RX J1605.3+3249 at Frequency of 111 MHz

Year: 2025

Type: article

Abstract: For the first time, pulsed radio emission from the RX J1605.3+3249 magnetar, 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 of $$S = 50{\kern 1pt} - {\kern 1pt} 100$$ mJy and the dispersion measure of $$DM = 4.7 \pm 0.5$$ pc/cm 3 have been measured.

Source: Astronomy Reports

DOI: 10.1134/s1063772925701756

Authors: A. E. Rodin, V. A. Fedorova

Institutions: P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Russian Academy of Sciences

Language: English

Topic: Pulsars and Gravitational Waves Research

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: hybrid

OpenAlex ID: W4411523408

FWCI:

Cites: 17

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Related to: 10