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Autor:
Agar, C. H., Weltevrede, P., Bondonneau, L., Grießmeier, J. -M., Hessels, J. W. T., Huang, W. J., Karastergiou, A., Keith, M. J., Kondratiev, V. I., Künsemöller, J., Li, D., Peng, B., Sobey, C., Stappers, B. W., Tan, C. M., Theureau, G., Wang, H. G., Zhang, C. M., Cecconi, B., Girard, J. N., Loh, A., Zarka, P.
We present radio observations of the most slowly rotating known radio pulsar PSR J0250+5854. With a 23.5 s period, it is close, or even beyond, the $P$-$\dot{P}$ diagram region thought to be occupied by active pulsars. The simultaneous observations w
Externí odkaz:
http://arxiv.org/abs/2109.00266