Comparing P‐Stars with Observations | Zendy

Paolo Cea | Zendy

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Comparing P‐Stars with Observations

Author(s) -

Paolo Cea

Publication year - 2008

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/524770

Subject(s) - stars , physics , astrophysics , k type main sequence star , neutron star , compact star , t tauri star , astronomy

P-stars are compact stars made of up and down quarks in $\beta$-equilibriumwith electrons in a chromomagnetic condensate. P-stars are able to account forcompact stars as well as stars with radius comparable with canonical neutronstars. We compare p-stars with different available observations. Our resultsindicate that p-stars are able to reproduce in a natural manner severalobservations from isolated and binary pulsars.Comment: 15 pages, 2 figures; accepted for publication in Astrophysical Journa

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