从三年的监测数据中寻找旋转无线电瞬变体

IF 5.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2024-08-27 DOI:10.1051/0004-6361/202449762
S. A. Tyul’bashev, M. A. Kitaeva, D. V. Pervoukhin, G. E. Tyul’basheva, E. A. Brylyakova, A. V. Chernosov, I. L. Ovchinnikov
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引用次数: 0

摘要

对旋转射电瞬变体(RRATs)的搜索是在 111 MHz 频率下进行的,通过大型相控阵(LPA)射电望远镜在 -9° < δ +42° 的偏角范围内进行日常观测。总共发现了 19 个新的 RRAT,其色散度量(DMs)为 2.5 至 72.6 pc cm-3。其中两个(J0408+28;J0440+35)与太阳的距离分别为 134 和 136 pc,是所有已知 RRAT 中距离最近的。
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Search for rotating radio transients in three years of monitoring data
The search for rotating radio transients (RRATs) was carried out at a frequency of 111 MHz, as daily observations carried out on the Large Phased Array (LPA) radio telescope at declinations of −9° < δ < +42°. Overall, 19 new RRATs were discovered for dispersion measures (DMs) from 2.5 to 72.6 pc cm−3. Estimates of the periods were obtained for three RRATs, with two of them (J0408+28; J0440+35) located at distances of 134 and 136 pc from Sun, placing them among the closest of all known RRATs.
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