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Discovery of a Pulsar-powered Bow Shock Nebula in the Small Magellanic Cloud Supernova Remnant DEMS5
Autor:
Alsaberi, Rami Z. E., Maitra, C., Filipovi'c, M. D., Bozzetto, L. M., Haberl, F., Maggi, P., Sasaki, M., Manjolovi'c, P., Velovi'c, V., Kavanagh, P., Maxted, N. I., Urovsevi'c, D., Rowell, G. P., Wong, G. F., For, B. -Q., O'Brien, A. N., Galvin, T. J., Staveley-Smith, L., Norris, R. P., Jarrett, T., Kothes, R., Luken, K. J., Hurley-Walker, N., Sano, H., Oni'c, D., Dai, S., Pannuti, T. G., Tothill, N. F. H., Crawford, E. J., Yew, M., Bojivci'c, I., D'enes, H., McClure-Griffiths, N., Gurovich, S., Fukui, Y.
We report the discovery of a new Small Magellanic Cloud Pulsar Wind Nebula (PWN) at the edge of the Supernova Remnant (SNR)-DEM S5. The pulsar powered object has a cometary morphology similar to the Galactic PWN analogs PSR B1951+32 and 'the mouse'.
Externí odkaz:
http://arxiv.org/abs/1903.03226