| The observed velocity distribution of young pulsars F Verbunt, A Igoshev, E Cator Astronomy & Astrophysics 608, A57, 2017 | 186 | 2017 |
| The Galactic distribution of X-ray binaries and its implications for compact object formation and natal kicks S Repetto, AP Igoshev, G Nelemans Monthly Notices of The Royal Astronomical Society 467 (1), 298-310, 2017 | 139 | 2017 |
| Evolution of neutron star magnetic fields AP Igoshev, SB Popov, R Hollerbach Universe 7 (9), 351, 2021 | 73 | 2021 |
| The demographics of neutron star–white dwarf mergers-Rates, delay-time distributions, and progenitors S Toonen, HB Perets, AP Igoshev, E Michaely, Y Zenati Astronomy & Astrophysics 619, A53, 2018 | 73 | 2018 |
| The observed velocity distribution of young pulsars–II. Analysis of complete PSRπ AP Igoshev Monthly Notices of the Royal Astronomical Society 494 (3), 3663-3674, 2020 | 49 | 2020 |
| Neutron star's initial spin period distribution AP Igoshev, SB Popov Monthly Notices of the Royal Astronomical Society 432 (2), 967-972, 2013 | 45 | 2013 |
| Combined analysis of neutron star natal kicks using proper motions and parallax measurements for radio pulsars and Be X-ray binaries AP Igoshev, M Chruslinska, A Dorozsmai, S Toonen Monthly Notices of the Royal Astronomical Society 508 (3), 3345-3364, 2021 | 37 | 2021 |
| Magnetic field decay in normal radio pulsars AP Igoshev, SB Popov Astronomische Nachrichten 336 (8‐9), 831-834, 2015 | 35 | 2015 |
| Modified pulsar current analysis: probing magnetic field evolution AP Igoshev, SB Popov Monthly Notices of the Royal Astronomical Society 444 (2), 1066-1076, 2014 | 35 | 2014 |
| Strong toroidal magnetic fields required by quiescent X-ray emission of magnetars AP Igoshev, R Hollerbach, T Wood, KN Gourgouliatos Nature Astronomy 5 (2), 145-149, 2021 | 33 | 2021 |
| Post-fall-back evolution of multipolar magnetic fields and radio pulsar activation AP Igoshev, JG Elfritz, SB Popov Monthly Notices of the Royal Astronomical Society 462 (4), 3689-3702, 2016 | 31 | 2016 |
| Distance and luminosity probability distributions derived from parallax and flux with their measurement errors-With application to the millisecond pulsar PSR J0218+ 4232 A Igoshev, F Verbunt, E Cator Astronomy & Astrophysics 591, A123, 2016 | 31 | 2016 |
| Initial periods and magnetic fields of neutron stars AP Igoshev, A Frantsuzova, KN Gourgouliatos, S Tsichli, L Konstantinou, ... Monthly Notices of the Royal Astronomical Society 514 (3), 4606-4619, 2022 | 27 | 2022 |
| 3D magnetothermal simulations of tangled crustal magnetic field in central compact objects AP Igoshev, KN Gourgouliatos, R Hollerbach, TS Wood The Astrophysical Journal 909 (2), 101, 2021 | 24 | 2021 |
| Wide binary companions to massive stars and their use in constraining natal kicks AP Igoshev, HB Perets Monthly Notices of the Royal Astronomical Society 486 (3), 4098-4113, 2019 | 24 | 2019 |
| Inferred time-scales for common envelope ejection using wide astrometric companions AP Igoshev, HB Perets, E Michaely Monthly Notices of the Royal Astronomical Society 494 (1), 1448-1462, 2020 | 23 | 2020 |
| How to make a mature accreting magnetar AP Igoshev, SB Popov Monthly Notices of the Royal Astronomical Society 473 (3), 3204-3210, 2018 | 23 | 2018 |
| Powering central compact objects with a tangled crustal magnetic field KN Gourgouliatos, R Hollerbach, AP Igoshev Monthly Notices of the Royal Astronomical Society 495 (2), 1692-1699, 2020 | 22 | 2020 |
| Testing the fossil field hypothesis: could strongly magnetized OB stars produce all known magnetars? EI Makarenko, AP Igoshev, AF Kholtygin Monthly Notices of the Royal Astronomical Society 504 (4), 5813-5828, 2021 | 20 | 2021 |
| Hyper-runaway and hypervelocity white dwarf candidates in Gaia Data Release 3: Possible remnants from Ia/Iax supernova explosions or dynamical encounters AP Igoshev, H Perets, N Hallakoun Monthly Notices of the Royal Astronomical Society 518 (4), 6223-6237, 2023 | 15 | 2023 |
Sergei B. PopovSternberg Astronomical Institute and ICTP (Trieste)在 sai.msu.ru 的电子邮件经过验证
