Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-22T11:41:19.217Z Has data issue: false hasContentIssue false
  • English
  • Français

Observability of isolated neutron stars at SRG/eROSITA

Published online by Cambridge University Press:  27 February 2023

Alena D. Khokhriakova Open the ORCID record for Alena D. Khokhriakova [Opens in a new window] ,
Anton V. Biryukov  and
Sergei B. Popov Open the ORCID record for Sergei B. Popov [Opens in a new window]
Alena D. Khokhriakova*
Affiliation:
Faculty of Physics, Moscow State University, Moscow, Russia Sternberg Astronomical Institute, Moscow State University, Moscow, Russia “Basis” foundation fellow, Moscow, Russia
Anton V. Biryukov
Affiliation:
Sternberg Astronomical Institute, Moscow State University, Moscow, Russia Kazan Federal University, Kazan, Russia
Sergei B. Popov
Affiliation:
Faculty of Physics, Moscow State University, Moscow, Russia Sternberg Astronomical Institute, Moscow State University, Moscow, Russia
*
email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A four-year sky survey with the use of the eROSITA telescope on board the Spektr-RG observatory will provide the best coverage in the soft (0.5–2 keV) and standard (2–10 keV) X-ray ranges, both in terms of sensitivity and angular resolution. We have analysed the possibility of detecting various types of isolated neutron stars with eROSITA. Among already known objects, eROSITA will be able to detect more than 160 pulsars, 21 magnetars, 7 central compact objects, all seven sources of the Magnificent Seven, and two other X-ray isolated neutron stars during the four-year survey mission.

Keywords

Stars: neutronpulsars: generalX-rays: stars
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S363: Neutron Star Astrophysics at the Crossroads: Magnetars and the Multimessenger Revolution , June 2020 , pp. 301 - 304
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

References

Becker, W. 2009, Ap&SSL, 357, 91 CrossRefGoogle Scholar
De Luca, A. 2017, Journal of Physics Conference Series, 932, 012006 Google Scholar
Igoshev, A.P. & Popov, S.B. 2018, MNRAS, 473, 3204 CrossRefGoogle Scholar
Khokhryakova, A. D., Biryukov, A. V., & Popov, S. B. 2021, Astronomy Reports, 65, 615 Google Scholar
Khokhryakova, A.D., Lyapina, D.A., & Popov, S.B. 2019, Astronomy Letters, 45, 120 CrossRefGoogle Scholar
Manchester, R.N., Hobbs, G.B., Teoh, A., & Hobbs, M. 2005, AJ, 129, 1993 CrossRefGoogle Scholar
Merloni, A., et al. 2012, arXiv e-prints, arXiv:1209.3114.Google Scholar
Olausen, S.A. & Kaspi, V.M. 2014, Astrophys. J. Suppl., 212, 6 CrossRefGoogle Scholar
Ostriker, J.P., Rees, M.J., & Silk, J. 1970, Astrophysical Letters, 6, 179 Google Scholar
Pires, A.M., Schwope, A.D., & Motch, C. 2017, Astron. Nachr., 338, 213 Google Scholar
Possenti, A., Cerutti, R., Colpi, M., & Mereghetti, S. 2002, A&A, 387, 993 CrossRefGoogle Scholar
Potekhin, A.Y., Chabrier, G., & Yakovlev, D.G. 1997, A&A, 323, 415 Google Scholar
Potekhin, A.Y., et al. 2020, MNRAS, 496, 5052 CrossRefGoogle Scholar
Schwope, A.D., Hasinger, G., Schwarz, R., Haberl, F., & Schmidt, M. 1999, A&A, 341, L51.Google Scholar
Shternin, P.S., et al. 2011, MNRAS, 412, L108 CrossRefGoogle Scholar
Shvartsman, V.G. 1971, SvA, 14, 662 CrossRefGoogle Scholar
Treves, A., Turolla, R., Zane, S., & Colpi, M. 2000, PASP, 112, 297 CrossRefGoogle Scholar