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PSR B1257+12, previously designated PSR 1257+12, alternatively designated PSR J1300+1240, [6] is a millisecond pulsar, 2,300 light-years (710 parsecs) from the Sun, in the constellation Virgo, rotating at about 161 times per second (faster than the blade of a blender). [1]
The main problem is that the resulting pulsar would be a radio pulsar, not the type of pulsar that PSR B1257+12 is. Thus, it is unlikely that this was how the planet formed. [11] The most widely accepted model for the planets around Lich is that they were a result of two white dwarfs merging. The white dwarfs would be in a binary orbit, with ...
Pulsar XP (also called the XP912) Improved model, with higher gross weight, powered by an 80 hp (60 kW) Rotax 912UL four-stroke powerplant and introduced in 1992 by Aero Designs. [2] Pulsar Series II Improved model, powered by a 100 hp (75 kW) Rotax 912ULS four-stroke or 115 hp (86 kW) Rotax 914 turbocharged powerplant and produced by SkyStar ...
Gamma ray and optical (visible light) light curves for the pulsar, adapted from Spolon et al. (2019) [3]. Vela is the brightest pulsar (at radio frequencies) in the sky and spins 11 times per second [4] (i.e. a period of 89.33 milliseconds—the shortest known at the time of its discovery) and the remnant from the supernova explosion is estimated to be travelling outwards at 1,200 km/s (750 mi ...
An intermediate-mass binary pulsar (IMBP) is a pulsar-white dwarf binary system with a relatively long spin period of around 10–200 ms consisting of a white dwarf with a relatively high mass of approximately . [7] The spin periods, magnetic field strengths, and orbital eccentricities of IMBPs are significantly larger than those of low mass binary pulsars (LMBPs). [7]
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