Dynamical friction of pulsars in globular clusters
Author:
Funder
National Natural Science Foundation of China
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://link.springer.com/content/pdf/10.1007/s10509-023-04208-z.pdf
Reference51 articles.
1. Abbate, F., Possenti, A., Ridolfi, A., et al.: Internal gas models and central black hole in 47 Tucanae using millisecond pulsars. Mon. Not. R. Astron. Soc. 481(1), 627–638 (2018). https://doi.org/10.1093/mnras/sty2298. arXiv:1808.06621 [astro-ph.HE]
2. Abbate, F., Possenti, A., Colpi, M., et al.: Evidence of nonluminous matter in the center of M62. Astrophys. J. Lett. 884(1), L9 (2019a). https://doi.org/10.3847/2041-8213/ab46c3. arXiv:1909.11091 [astro-ph.HE]
3. Abbate, F., Spera, M., Colpi, M.: Intermediate mass black holes in globular clusters: effects on jerks and jounces of millisecond pulsars. Mon. Not. R. Astron. Soc. 487(1), 769–781 (2019b). https://doi.org/10.1093/mnras/stz1330. arXiv:1905.05209 [astro-ph.HE]
4. Aceves, H., Colosimo, M.: Dynamical friction in stellar systems: an introduction. arXiv e-prints. arXiv:physics/0603066 [physics.class-ph] (2006)
5. Alessandrini, E., Lanzoni, B., Ferraro, F.R., et al.: Investigating the mass segregation process in globular clusters with blue straggler stars: the impact of dark remnants. Astrophys. J. 833(2), 252 (2016). https://doi.org/10.3847/1538-4357/833/2/252. arXiv:1610.04562 [astro-ph.GA]
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