| Entropy, complexity and disequilibrium in compact stars MGB De Avellar, JE Horvath Physics Letters A 376 (12-13), 1085-1089, 2012 | 60 | 2012 |
| Information theoretical methods as discerning quantifiers of the equations of state of neutron stars MGB De Avellar, RA De Souza, JE Horvath, DM Paret Physics Letters A 378 (47), 3481-3487, 2014 | 54 | 2014 |
| Time lags of the kilohertz quasi-periodic oscillations in the low-mass X-ray binaries 4U 1608--52 and 4U 1636--53 M de Avellar, M Méndez, A Sanna, J Horvath Monthly Notices of the Royal Astronomical Society, 2013 | 47 | 2013 |
| Neutron stars in f (ℛ, T) gravity using realistic equations of state in the light of massive pulsars and GW170817 R Lobato, O Lourenço, P Moraes, CH Lenzi, M De Avellar, W De Paula, ... Journal of Cosmology and Astroparticle Physics 2020 (12), 039, 2020 | 36 | 2020 |
| Microbial habitability of Europa sustained by radioactive sources T Altair, MGB de Avellar, F Rodrigues, D Galante Scientific reports 8 (1), 260, 2018 | 29 | 2018 |
| A light strange star in the remnant HESS J1731− 347: Minimal consistency checks JE Horvath, LS Rocha, LM de Sá, P Moraes, LG Barão, MGB de Avellar, ... Astronomy & Astrophysics 672, L11, 2023 | 26 | 2023 |
| Self-bound models of compact stars and recent mass-radius measurements MGB de Avellar, JE Horvath, L Paulucci Physical Review D 84 (4), 043004, 2011 | 26 | 2011 |
| Exact solutions of a model for strange stars with interacting quarks LS Rocha, A Bernardo, MGB de Avellar, JE Horvath Astronomische Nachrichten 340 (1-3), 180-183, 2019 | 21 | 2019 |
| Exact solutions for compact stars with CFL quark matter LS Rocha, A Bernardo, MGB De Avellar, JE Horvath International Journal of Modern Physics D 29 (07), 2050044, 2020 | 20 | 2020 |
| Kilohertz QPOs in low-mass X-ray binaries as oscillation modes of tori around neutron stars–I MGB de Avellar, O Porth, Z Younsi, L Rezzolla Monthly Notices of the Royal Astronomical Society 474 (3), 3967-3975, 2018 | 20 | 2018 |
| Neutron stars in f(ℛ, 𝒯) 𝑓 ℛ 𝒯 f (\mathcal {R, T}) italic_f (caligraphic_R, caligraphic_T)) gravity using realistic equations of state in the light of massive pulsars and GW170817 R Lobato, O Lourenço, P Moraes, CH Lenzi, M de Avellar, W de Paula, ... JCAP 12, 039, 2020 | 19 | 2020 |
| Exact and quasi-exact models of strange stars MGB De Avellar, JE Horvath International Journal of Modern Physics D 19 (12), 1937-1955, 2010 | 17 | 2010 |
| Phase lags of quasi-periodic oscillations across source states in the low-mass X-ray binary 4U 1636–53 MGB De Avellar, M Méndez, D Altamirano, A Sanna, G Zhang Monthly Notices of the Royal Astronomical Society 461 (1), 79-92, 2016 | 15 | 2016 |
| The amplitude of the kilohertz quasi-periodic oscillations in 4U 1636–53 in the frequency-energy space EM Ribeiro, M Méndez, MGB de Avellar, G Zhang, K Karpouzas Monthly Notices of the Royal Astronomical Society 489 (4), 4980-4991, 2019 | 13 | 2019 |
| Redback/Black Widow Systems as progenitors of the highest neutron star masses and low-mass Black Holes JE Horvath, A Bernardo, LS Rocha, R Valentim, P Moraes, ... arXiv preprint arXiv:2006.06398, 2020 | 9 | 2020 |
| Birth events, masses and the maximum mass of Compact Stars JE Horvath, LS Rocha, ALC Bernardo, MGB de Avellar, R Valentim Astrophysics in the XXI Century with Compact Stars, 1-51, 2023 | 8 | 2023 |
| The distribution of neutron star masses LS Rocha, A Bernardo, JE Horvath, R Valentim, MGB de Avellar Astronomische Nachrichten 340 (9-10), 957-963, 2019 | 8 | 2019 |
| Statistical measure of complexity in compact stars with global charge neutrality RA de Souza, MGB de Avellar, JE Horvath arXiv preprint arXiv:1308.3519, 2013 | 8 | 2013 |
| Neutron stars origins and masses JE Horvath, LS Rocha, A Bernardo, R Valientim, MGB de Avellar Astronomische Nachrichten 342 (1-2), 294-299, 2021 | 5 | 2021 |
| Natural radioactive environments as sources of local disequilibrium for the emergence of life T Altair, LM Sartori, F Rodrigues, MGB de Avellar, D Galante Astrobiology 20 (12), 1489-1497, 2020 | 5 | 2020 |
Mariano MendezProfessor of High-Energy Astrophysics, University of Groningen在 astro.rug.nl 的电子邮件经过验证
