DescriptionTOV solution neutron quark star mass radius diagram.png
English: TOV solutions on the mass-radius diagram, for npeμ nuclear matter (Skyrme-Lyon model by F. Douchin, P. Haensel, Astron. Astrophys. 380, 151 [2001]) ploted with red line and bare quark matter star, described by MIT bag model (coupling constant alpha=0.17, bag constant B=60 MeV/fm^3, quark mass ms=200 MeV) ploted with blue line. TOV limit are marked with dots.
Polski: Rozwiązania równań TOV na diagramie masa-promień dla równania stanu gwiazdy neutronowej otrzymanego przez F. Douchina i P. Haensela (skład npeμ, model Skyrme-Lyon, Astron. Astrophys. 380, 151 [2001]) oznaczone linią czerwoną, oraz dla równania stanu nagiej gwiazdy kwarkowej (modelu "worka", o stałej sprzężenia alpha=0.17, stałej worka B=60 MeV/fm^3, masie kwarku dziwnego ms=200MeV) oznaczone niebieską linią. Granice TOV zaznaczone kropkami.
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{{Information |Description={{en|1=TOV solutions on the mass-radius diagram, for npeμ nuclear matter (Skyrme-Lyon model by F. Douchin, P. Haensel, Astron. Astrophys. 380, 151 [2001]) ploted with red line and bare quark matter star, described by MIT bag
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