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Иш: Constraining <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si170.svg" display="inline" id="d1e5067"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">R</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi mathvariant="script">L</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> </mml:msub> <mml:mo>,</mml:mo> <mml:mi mathvariant="script">T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity with NICER/NuSTAR observations of X-ray Pulsars
THE MASS AND RADIUS OF THE NEUTRON STAR IN EXO 1745–248
Feryal Özel, Tolga Güver, Dimitrios Psaltis
Мақола20092 иқтибосABITidal forces and fragmentation of self-gravitating compact objects
A. Di Prisco, E. Fuenmayor, L. Herrera +1
Мақола19942 иқтибосABIA stellar census in globular clusters with MUSE: Binaries in NGC 3201
Benjamin Giesers, Sebastian Kamann, Stefan Dreizler +8
Мақола20192 иқтибосABIDymnikova-Schwinger GUP-corrected wormholes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si18.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mo>(</mml:mo> <mml:mi>R</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mi>L</mml:mi> <mml:mi>m</mml:mi> </mml:msub> <mml:mo>,</mml:mo> <mml:mi>T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:math> gravity
Abdelghani Errehymy, Bobur Turimov, A. Syzdykova +3
Мақола20252 иқтибосABI