LOFAR Detection of 110–188 MHz Emission and Frequency-dependent Activity from FRB 20180916B

The object FRB 20180916B is a well-studied repeating fast radio burst source. Its proximity (∼150 Mpc), along with detailed studies of the bursts, has revealed many clues about its nature, including a 16.3 day periodicity in its activity. Here we report on the detection of 18 bursts using LOFAR at 1...

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Veröffentlicht in:	Astrophysical journal. Letters 2021-04, Vol.911 (1), p.L3
Hauptverfasser:	Pleunis, Z., Michilli, D., Bassa, C. G., Hessels, J. W. T., Naidu, A., Andersen, B. C., Chawla, P., Fonseca, E., Gopinath, A., Kaspi, V. M., Kondratiev, V. I., Li, D. Z., Bhardwaj, M., Boyle, P. J., Brar, C., Cassanelli, T., Gupta, Y., Josephy, A., Karuppusamy, R., Keimpema, A., Kirsten, F., Leung, C., Marcote, B., Masui, K. W., Mckinven, R., Meyers, B. W., Ng, C., Nimmo, K., Paragi, Z., Rahman, M., Scholz, P., Shin, K., Smith, K. M., Stairs, I. H., Tendulkar, S. P.
Format:	Artikel
Sprache:	eng
Schlagworte:	Binary stars Circular polarization Companion stars Emission Faraday effect Gamma rays Linear polarization LOFAR Neutron stars Optical analysis Optical thickness Periodic variations Polarization Radio bursts Sciences of the Universe
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