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  • Cygnus X-1 — For other uses, see Cygnus X 1 (disambiguation). HDE 226868 HDE 226868 (not shown) is located next to the star η (lower center) in this map of constellation Cygnus …   Wikipedia

  • Wolverhampton Wanderers F.C. — Football club infobox clubname = Wolverhampton Wanderers fullname = Wolverhampton Wanderers Football Club nickname = Wolves The Wanderers founded = 1877 (as St. Luke s) ground = Molineux Stadium Wolverhampton England capacity = 28,525 CEO = Jez… …   Wikipedia

  • Pentaceratops — Taxobox name = Pentaceratops fossil range = Late Cretaceous image width = 250px | regnum = Animalia phylum = Chordata classis = Sauropsida superordo = Dinosauria ordo = Ornithischia subordo = Ceratopsia familia = Ceratopsidae subfamilia =… …   Wikipedia

  • Tolman-Oppenheimer-Volkoff limit — The Tolman Oppenheimer Volkoff (TOV) limit is an upper bound to the mass of stars composed of neutron degenerate matter (neutron stars). It is analogous to the Chandrasekhar limit for white dwarf stars.The limit was computed by J. Robert… …   Wikipedia

  • Tolman-Oppenheimer-Volkoff equation — In astrophysics, the Tolman Oppenheimer Volkoff (TOV) equation constrains the structure of a spherically symmetric body of isotropic material which is in static gravitational equilibrium, as modelled by general relativity. The equation… …   Wikipedia

  • Type II supernova — The expanding remnant of SN 1987A, a Type II P supernova in the Large Magellanic Cloud. NASA image. A Type II supernova (plural: supernovae) results from the rapid collapse and violent explosion of a massive star. A star must have at least 9… …   Wikipedia

  • 2007 BWF Grand Prix Gold and Grand Prix — The 2007 BWF Grand Prix Gold and Grand Prix was the inaugural season of BWF Grand Prix Gold and Grand Prix under the new tournament structure introduced by Badminton World Federation (BWF). It was held from February 27 and will end on December 12 …   Wikipedia

  • Quark-Stern — Ein Quarkstern, auch Seltsamer genannt, ist ein theoretisch möglicher Endzustand der Sternentwicklung vor einem Schwarzen Loch. Mit dem Verbrauch seines nuklearen Brennmaterials (Kernfusion) wird die Materie eines Sterns durch die Gravitation… …   Deutsch Wikipedia

  • Seltsamer — Ein Quarkstern, auch Seltsamer genannt, ist ein theoretisch möglicher Endzustand der Sternentwicklung vor einem Schwarzen Loch. Mit dem Verbrauch seines nuklearen Brennmaterials (Kernfusion) wird die Materie eines Sterns durch die Gravitation… …   Deutsch Wikipedia

  • TOV — Die Tolman Oppenheimer Volkoff Grenze (TOV) ist eine obere Schranke für die Masse stellarer Objekte, die aus entarteter Neutronenmaterie bestehen (Neutronensterne). Sie ist Analog zur Chandrasekhar Grenze für weiße Zwerge. Die Grenze wurde… …   Deutsch Wikipedia

  • Tolman–Oppenheimer–Volkoff equation — In astrophysics, the Tolman–Oppenheimer–Volkoff (TOV) equation constrains the structure of a spherically symmetric body of isotropic material which is in static gravitational equilibrium, as modelled by general relativity. The equation[1] is Here …   Wikipedia

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