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Early accretion onset in long-period isolated pulsars

Published online by Cambridge University Press:  27 February 2024

M.D. Afonina Open the ORCID record for M.D. Afonina [Opens in a new window] ,
A.V. Biryukov  and
S.B. Popov
M.D. Afonina*
Affiliation:
Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetskij pr. 13, 119234, Moscow, Russia Faculty of Physics, Lomonosov Moscow State University, 1/2 Leninskie Gory, Moscow, 119991, Russia
A.V. Biryukov
Affiliation:
Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetskij pr. 13, 119234, Moscow, Russia Faculty of Physics, HSE University, 21/4 Staraya Basmannaya str., Moscow, 105066, Russia Kazan Federal University, 18 Kremlyovskaya str., Kazan, 420008, Russia
S.B. Popov
Affiliation:
Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetskij pr. 13, 119234, Moscow, Russia ICTP-Abdus Salam International Center for Theoretical Physics, Strada Costiera 11, I-34151 Trieste, Italy
*
Corresponding author: M.D. Afonina; Email: afonina.md19@physics.msu.ru.
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Abstract

We model long-term magneto-rotational evolution of isolated neutron stars (INSs) with long initial spin periods. This analysis is motivated by the recent discovery of young long-period neutron stars (NSs) observed as periodic radio sources: PSR J0901-4046, GLEAM-X J1627-52, and GPM J1839-10. Our calculations demonstrate that for realistically rapid spin-down during the propeller stage INSs with velocities ${\lesssim}100$ km s$^{-1}$ and assumed long initial spin periods can reach the stage of accretion from the interstellar medium within at most a few billion years as they are born already at the propeller stage or sufficiently close to the critical period of the ejector-propeller transition. If NSs with long initial spin periods form a relatively large fraction of all Galactic NSs then the number of isolated accretors is substantially larger than it has been predicted by previous studies.

Keywords

accretionBondi accretioncompact objectsneutron starspulsars
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 41 , 2024 , e014
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of Astronomical Society of Australia

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References

Afonina, M. D., Biryukov, A. V., & Popov, S. B. 2023, arXiv e-prints (September): arXiv:2309.12080. https://doi.org/10.48550/arXiv.2309.12080 CrossRefGoogle Scholar
Aguilera, D. N., J. A., & Miralles, J. A. 2008, A&A, 486, 255 CrossRefGoogle Scholar
Andrews, J. J., Taggart, K., & Foley, R. 2022, arXiv e-prints (july): arXiv:2207.00680. https://doi.org/10.48550/arXiv.2207.00680 CrossRefGoogle Scholar
Avakyan, A., Neumann, M., Zainab, A., Doroshenko, V., Wilms, J. and Santangelo, A. 2023, A&A, 675, A199 CrossRefGoogle Scholar
Beniamini, P., Wadiasingh, Z., Hare, J., Rajwade, K. M., Younes, G. & van der Horst, A. J. 2023, MNRAS, 520, 1872 CrossRefGoogle Scholar
Beskin, V. S. 2018, Phys. Uspekhi, 61, 353 CrossRefGoogle Scholar
Beskin, V. S., & Eliseeva, S. A. 2005, Astron. Lett., 31, 263 CrossRefGoogle Scholar
Blondin, J. M., & Raymer, E. 2012, ApJ, 752, 30 CrossRefGoogle Scholar
Boldin, P. A., & Popov, S. B. 2010, MNRAS, 407, 1090 CrossRefGoogle Scholar
Bondi, H., & Hoyle, F. 1944, MNRAS, 104, 273 CrossRefGoogle Scholar
Caleb, M., Heywood, I., Rajwade, K., Malenta, M., Stappers, B. W., Barr, E., Chen, W., et al. 2022, Nature Astron., 6, 828 CrossRefGoogle Scholar
Davidson, K., & Ostriker, J. P. 1973, ApJ, 179, 585 CrossRefGoogle Scholar
Davies, R. E., Fabian, A. C., & Pringle, J. E. 1979, MNRAS, 186, 779 CrossRefGoogle Scholar
Davies, R. E., & Pringle, J. E. 1981, MNRAS, 196, 209 CrossRefGoogle Scholar
Fortin, F., García, F., Bunzel, A. S., & Chaty, S. 2023, A&A, 671, A149.Google Scholar
Gourgouliatos, K. N., & Cumming, A. 2014, MNRAS, 438, 1618 CrossRefGoogle Scholar
Gourgouliatos, K. N., & Cumming, A. 2014a, Phys. Rev. Lett., 112, 171101 CrossRefGoogle Scholar
Hurley-Walker, N., Rea, N., McSweeney, S. J., Meyers, B. W., Lenc, E., Heywood, I., Hyman, S. D., et al. 2023, Nature, 619, 487 CrossRefGoogle Scholar
Hurley-Walker, N., Zhang, X., Bahramian, A., McSweeney, S. J., O’Doherty, T. N., Hancock, P. J., Morgan, J. S., Anderson, G. E., Heald, G. H., & Galvin, T. J. 2022, Nature, 601, 526 CrossRefGoogle Scholar
Igoshev, A. P., Popov, S. B., & Hollerbach, R. 2021, Universe, 7, 351 CrossRefGoogle Scholar
Illarionov, A. F., & Sunyaev, R. A. 1975, A&A, 39, 185 Google Scholar
Klessen, R. S., & Glover, S.C.O. 2016, in Saas-fee advanced course, edited by Revaz, Y., Jablonka, P., Teyssier, R., & Mayer, L., 43, 85 CrossRefGoogle Scholar
Lam, C. Y., Lu, J. R. Jr., Hosek, M. W., Dawson, W. A., & Golovich, N. R. 2020, ApJ, 889, 31.Google Scholar
Lipunov, V. M., & Popov, S. B., 1995, AZh, 72, 711.Google Scholar
Lipunov, V. M. 1992. Astrophysics of Neutron Stars, Astronomy and Astrophysics Library, Springer-Verlag, Berlin HeidelbergGoogle Scholar
Liu, Q. Z., van Paradijs, J., & van den Heuvel, E. P. J. 2007. A&A, 469, 807 CrossRefGoogle Scholar
Lyutikov, M. 2023, MNRAS, 520, 4315 CrossRefGoogle Scholar
Manchester, R. N., Hobbs, G. B., Teoh, A., & Hobbs, M. 2005, AJ, 129, 1993 CrossRefGoogle Scholar
Mazeh, T., Faigler, S., Bashi, D., Shahaf, S., Davidson, N., Green, M., Gomel, R., et al. 2022, MNRAS, 517, 4005 CrossRefGoogle Scholar
Mroz, P., Udalski, A., Wyrzykowski, L., Skowron, J., Poleski, R., Szymanski, M., Soszynski, I., & Ulaczyk, K. 2021, arXiv e-prints, arXiv:2107.13697. https://doi.org/10.48550/arXiv.2107.13697 CrossRefGoogle Scholar
Neumann, M., Avakyan, A., Doroshenko, V., & Santangelo, A. 2023, arXiv e-prints, (March): arXiv:2303.16137. https://doi.org/10.48550/arXiv.2303.16137 CrossRefGoogle Scholar
Ostriker, J. P., Rees, M. J., & Silk, J. 1970, Astrophys. Lett., 6, 179 Google Scholar
Philippov, A., Tchekhovskoy, A., & Li, J. G. 2014, MNRAS, 441, 1879 CrossRefGoogle Scholar
Pons, J. A., & Viganò, D. 2019, Living Rev. Computat. Astrophys., 5, 3 CrossRefGoogle Scholar
Popov, S. B., Colpi, M., Treves, A., Turolla, R., Lipunov, V. M. and Prokhorov, M. E. 2000, ApJ, 530, 896 CrossRefGoogle Scholar
Popov, S. B., Postnov, K. A., & Shakura, N. I. 2015, MNRAS, 447, 2817 CrossRefGoogle Scholar
Popov, S. B., Prokhorov, M. E., Khoperskov, A. V., & Lipunov, V. M. 2001, arXiv e-prints (October): astroph/0110022. https://doi.org/10.48550/arXiv.astro-ph/0110022.Google Scholar
Popov, S. B., & Turolla, R. 2012, Ap&SS, 341, 457 CrossRefGoogle Scholar
Popov, S. B. 2023, Universe, 9, 273 CrossRefGoogle Scholar
Prasanna, T., Coleman, M. S. B., Raives, M. J., & Thompson, T. A. 2022, MNRAS, 517, 3008 CrossRefGoogle Scholar
Prokhorov, M. E., Popov, S. B., & Khoperskov, A. V. 2002, A&A, 381, 1000 CrossRefGoogle Scholar
Ronchi, M., Rea, N., Graber, V., & Hurley-Walker, N. 2022, ApJ 934: 184 CrossRefGoogle Scholar
Rozwadowska, K., Vissani, F., & Cappellaro, E. 2021, New A 83, 101498 CrossRefGoogle Scholar
Shakura, N., Postnov, K., Kochetkova, A., & Hjalmarsdotter, L. 2012, MNRAS, 420, 216 CrossRefGoogle Scholar
Shakura, N. I. 1975, Soviet Astron. Lett., 1, 223 Google Scholar
Shakura, N. I., Postnov, K. A., Kochetkova, A. Yu., Hjalmarsdotter, L., Sidoli, L., & Paizis, A. 2015, AR, 59, 645 CrossRefGoogle Scholar
Shvartsman, V. F. 1970, Soviet Ast., 14, 527 CrossRefGoogle Scholar
Shvartsman, V. F. 1971, Soviet Ast., 14, 662 CrossRefGoogle Scholar
Spitkovsky, A. 2006, ApJ, 648, L51 CrossRefGoogle Scholar
Toropina, O. D., Romanova, M. M., & Lovelace, R. V. E. 2012, MNRAS 420, 810 CrossRefGoogle Scholar
Treves, A., Turolla, R., Zane, S., & Colpi, M. 2000, PASP, 112, 297 CrossRefGoogle Scholar
Turner, M. L., Rutledge, R. E., Letcavage, R., Shevchuk, A. S. H., & Fox, D. B. 2010, ApJ, 714, 1424 CrossRefGoogle Scholar