Neutron star radii and crusts: uncertainties and unified equations of state M Fortin, C Providência, AR Raduta, F Gulminelli, JL Zdunik, P Haensel, ... Physical Review C 94 (3), 035804, 2016 | 327 | 2016 |
GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability T Malik, N Alam, M Fortin, C Providência, BK Agrawal, TK Jha, B Kumar, ... Physical Review C 98 (3), 035804, 2018 | 287 | 2018 |
Hypernuclei and massive neutron stars M Fortin, SS Avancini, C Providência, I Vidaña Physical Review C 95 (6), 065803, 2017 | 131 | 2017 |
Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation N Alam, BK Agrawal, M Fortin, H Pais, C Providência, AR Raduta, ... Physical Review C 94 (5), 052801, 2016 | 96 | 2016 |
Neutron stars with hyperon cores: stellar radii and equation of state near nuclear density M Fortin, JL Zdunik, P Haensel, M Bejger Astronomy & Astrophysics 576, A68, 2015 | 85 | 2015 |
Rotating neutron stars with exotic cores: masses, radii, stability P Haensel, M Bejger, M Fortin, L Zdunik The European Physical Journal A 52, 1-21, 2016 | 67 | 2016 |
Relativistic hypernuclear compact stars with calibrated equations of state M Fortin, AR Raduta, S Avancini, C Providência Physical Review D 101 (3), 034017, 2020 | 64 | 2020 |
Thermalization time and specific heat of the neutron stars crust M Fortin, F Grill, J Margueron, D Page, N Sandulescu Physical Review C 82 (6), 065804, 2010 | 61 | 2010 |
Neutron star properties and the equation of state for the core JL Zdunik, M Fortin, P Haensel Astronomy & Astrophysics 599, A119, 2017 | 59 | 2017 |
Hyperons in hot dense matter: what do the constraints tell us for equation of state? M Fortin, M Oertel, C Providência Publications of the Astronomical Society of Australia 35, 2018 | 53 | 2018 |
Hyperonic stars and the nuclear symmetry energy C Providência, M Fortin, H Pais, A Rabhi Frontiers in Astronomy and Space Sciences 6, 13, 2019 | 51 | 2019 |
Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars M Bejger, D Blaschke, P Haensel, JL Zdunik, M Fortin Astronomy & Astrophysics 600, A39, 2017 | 47 | 2017 |
Thermal states of neutron stars with a consistent model of interior M Fortin, G Taranto, GF Burgio, P Haensel, HJ Schulze, JL Zdunik Monthly Notices of the Royal Astronomical Society 475 (4), 5010-5022, 2018 | 44 | 2018 |
Theia: Faint objects in motion or the new astrometry frontier C Boehm, A Krone-Martins, A Amorim, G Anglada-Escudé, A Brandeker, ... arXiv preprint arXiv:1707.01348, 2017 | 39 | 2017 |
Fundamental physics and the absence of sub-millisecond pulsars B Haskell, JL Zdunik, M Fortin, M Bejger, R Wijnands, A Patruno Astronomy & Astrophysics 620, A69, 2018 | 37 | 2018 |
Thermal evolution of relativistic hyperonic compact stars with calibrated equations of state M Fortin, AR Raduta, S Avancini, C Providência Physical Review D 103 (8), 083004, 2021 | 33 | 2021 |
Influence of the crust on the neutron star macrophysical quantities and universal relations L Suleiman, M Fortin, JL Zdunik, P Haensel Physical Review C 104 (1), 015801, 2021 | 29 | 2021 |
Faint objects in motion: the new frontier of high precision astrometry F Malbet, C Boehm, A Krone-Martins, A Amorim, G Anglada-Escudé, ... Experimental Astronomy 51, 845-886, 2021 | 28 | 2021 |
Empirical constraints on the high-density equation of state from multimessenger observables M Ferreira, M Fortin, T Malik, BK Agrawal, C Providência Physical Review D 101 (4), 043021, 2020 | 28 | 2020 |
Accurate Ray-tracing of Realistic Neutron Star Atmospheres for Constraining Their Parameters FH Vincent, M Bejger, A Różańska, O Straub, T Paumard, M Fortin, ... The Astrophysical Journal 855 (2), 116, 2018 | 24 | 2018 |