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- W2963218921 abstract "Abstract The soft gamma repeater SGR 1900+14 was observed in Pushchino observatory since 1988 December using BSA radio telescope operating at 111 MHz. We have detected the pulsed radio emission (Shitov 1999) with the same 5.16 s period that was reported earlier for this object (Hurley et al. 1998). The timing analysis has shown that this new radio pulsar PSR J1907+0919 associated with SGR 1900+14 has a superstrong magnetic field, which is 8.1 · 10 14 G, thereby confirming that it is a ”magnetar” (Duncan & Thompson 1992; Kouveliotou et al. 1999). The dispersion measure of PSR J1907+0919 is 281.4(9) pc · cm −3 which gives an estimate of the pulsar’s distance as about 5.8 kpc." @default.
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- W2963218921 date "2000-01-01" @default.
- W2963218921 modified "2023-09-25" @default.
- W2963218921 title "Low Frequency Radio Emission of Pulsar PSR J1907+0919 Associated with the Magnetar SGR1900+14" @default.
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- W2963218921 doi "https://doi.org/10.1017/s025292110006098x" @default.
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