7/4/2023 0 Comments Cassiopeia gg![]() Alternatively, the observed radiation may be interpreted as emitted by a compact object (more likely, a black hole) accreting from a residual disk or from a late-type dwarf in a close binary. Such temperatures are consistent with the standard models of neutron star cooling. Home Champions MSI 2023 Kick-off Esports.op.gg Region Europe West Download Now Experience the fast speed of OP.GG for Desktop Real-time Auto Rune Setting OP Champions, Team Comps, and More Latest Meta and OP. ![]() Ranking 6th best mid laner for 11.19, placing Build 11.19 Cassiopeia in our C-Tier rankings. Among several possible interpretations, we favor a model of a strongly magnetized neutron star with magnetically confined hydrogen or helium polar caps (Tinfinitypc approximately 2.8 MK, Rpc approximately 1 km) on a cooler iron surface (Tinfinitys approximately 1.7 MK). Cassiopeia builds using machine learning. An upper limit on the (gravitationally redshifted) surface temperature is Tinfinitys<1.9-2.3 MK, depending on the chemical composition of the surface and the star's radius. One cannot exclude, however, the possibility that the observed emission originates from hot spots on a cooler neutron star surface. Fits with the neutron star atmosphere models increase the radius and reduce the temperature, but these parameters are still substantially different from those expected for a young neutron star. The inferred radii are too small, and the temperatures too high, for the radiation to be interpreted as emitted from the whole surface of a uniformly heated neutron star. One can fit the spectrum equally well with a blackbody model with T=6-8 MK, R=0.2-0.5 km, and Lbol=&parl0 1.4-1.9&parr0 x1033 ergs s-1. The power-law index is higher, and the luminosity lower, than those observed from very young pulsars. The power-law fit yields the photon index gamma=2.6-4.1, and luminosity L(0.1-5.0 keV&parr0 =&parl0 2-60&parr0 x1034 ergs s-1 for d=3.4 kpc. Because of the small number of photons detected, different spectral models can fit the observed spectrum. The analysis of these data does not show statistically significant variability of the source. There's also an external enclosure with to 8TB drives for backup.The central pointlike X-ray source of the Cassiopeia A supernova remnant was discovered in the Chandra first light observation and found later in the archival ROSAT and Einstein images. For data there's a few Western Digital Red HHD's. The main drive is a 250GB Samsung Evo 850 m.2 SSD for the O/S. Plus, if do get one of the higher core count Zen 2 CPU's the headroom will be nice for overclocking. So, I found a deal on an HX750i and decided to just use them since nobody seemed interested in buying them. However, I had the custom sleeved cables from my last main rig that work for the HXi PSU's. I went with the 760 because it was cheap and is compatible with UEFI as well. There's no integrated graphics on the 2600, and even if there were I wouldn't want it using system memory, I carried the EVGA GTX 760 SC over from the last build. The RAM is just some standard G.Skill Trident Z, non-RGB. However, I wanted to have the option to get a Zen 2 CPU and not be limited by the power delivery. I would have gotten an R7, but decided that I might want to get the 12 core 3900X or maybe even the 16 core, because. I wanted something that could handle transcoding as well as encoding. I would like to swap the Meshify S2 front panel on to this though. Granted the window is nice to be able to see diagnostic LED's and the current temp without even turning on the screen. Otherwise this case is overkill since it's sitting in my mechanical room and I don't really see it. This is the system I use for my dedicated file/media server.įor the case I went with a Fractal Define R6. ![]()
0 Comments
Leave a Reply. |