She was transformed into a half-snake creature by dark magic and now seeks a cure for her curse, while also using her powers to further her family’s goals. LoreĬassiopeia is a member of the wealthy and powerful Du Couteau family in the city-state of Noxus. To counter her, it is important to stay out of her poison range and to focus on disrupting her sustained damage. CountersĬassiopeia can struggle against enemies who can gap-close and burst her down quickly, such as Zed or LeBlanc. She also pairs well with allies who can protect her and peel for her, such as Lulu or Janna. Cassiopeia SynergiesĬassiopeia works well with allies who can provide additional crowd control or engage, such as Sejuani or Malphite. She can also choose to run Inspiration secondary for more sustain. In the rune tree, Cassiopeia typically runs either Conqueror or Dark Harvest for more damage output. She can also opt for items that provide additional survivability, such as Zhonya’s Hourglass or Banshee’s Veil. Cassiopeia BuildĬassiopeia benefits from items that increase her ability power and mana sustain, such as Luden’s Echo or Seraph’s Embrace. She also has the ability to slow and stun enemies with her ultimate, which can help her team secure kills or escape dangerous situations. Cassiopeia is a mid-lane mage in “League of Legends” known for her sustained damage output and crowd control abilities.Ĭassiopeia is a mage who excels at dealing sustained damage to enemies with her poison abilities. 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.Build, runes, synergies, counters, lore. Such temperatures are consistent with the standard models of neutron star cooling. 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). 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. 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.
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