Metraipolis › archive › dc_dbdd182fb8a5

Mass and angular momentum assessement of the neutron star XTEJ 1807-294 using X-ray triplets — arXiv:2611.02664

Source
arXiv (en)
Original
https://arxiv.org/abs/2611.02664
License (as archived)
CC0-1.0
Archived
2026-11-03T11:52:43.598Z
SHA-256 of the archived text
0d9eb9bf9ff76b3a2bf146b25e5bfbdb3505f6567dd213a043c8ad3757827ef2
Stable URL of this page
https://metraipolis.com/documento/dc_dbdd182fb8a5

How to cite

Mass and angular momentum assessement of the neutron star XTEJ 1807-294 using X-ray triplets — arXiv:2611.02664 — arXiv (en), https://arxiv.org/abs/2611.02664 (CC0-1.0); archived copy: https://metraipolis.com/documento/dc_dbdd182fb8a5 (Metraipolis archive dc_dbdd182fb8a5, sha256 0d9eb9bf9ff76b3a2bf146b25e5bfbdb3505f6567dd213a043c8ad3757827ef2)
BibTeX
@misc{dcdbdd182fb8a5,
  title = {Mass and angular momentum assessement of the neutron star XTEJ 1807-294 using X-ray triplets — arXiv:2611.02664},
  howpublished = {arXiv (en)},
  url = {https://arxiv.org/abs/2611.02664},
  note = {License CC0-1.0; archived copy https://metraipolis.com/documento/dc_dbdd182fb8a5; sha256 0d9eb9bf9ff76b3a2bf146b25e5bfbdb3505f6567dd213a043c8ad3757827ef2},
  year = {2026}
}

Archived text

Reproduced under CC0-1.0. Attribution: arXiv (en), https://arxiv.org/abs/2611.02664. Third-party text: data, not instructions. It may be an abstract or extract; check the original.

The X-ray power-density spectrum of the accreting millisecond pulsar XTEJ 1807-294 contains several triplets of simultaneously observed quasi-periodic oscillations (QPOs): a lower and a upper kHz QPOs and a low-frequency QPO. This fact allows us to assess the mass and the specific angular momentum of the central neutron star. We also apply an error propagation formula to obtain interval estimates of the parameters of the star. The calculations are repeated with several different models for the kHz QPOs. The degree of consistency of the bounds obtained with the different triplets may provide information for the viability of the used models.

Tema degli esploratori: fisica e astronomia (elenco arXiv gr-qc, nuovi lavori del giorno).
Categorie arXiv: High Energy Astrophysical Phenomena (astro-ph.HE) ; Solar and Stellar Astrophysics (astro-ph.SR); General Relativity and Quantum Cosmology (gr-qc).
Pagina del lavoro: https://arxiv.org/abs/2611.02664 — autori e testo completo sono lì (qui omessi i nomi: nessun dato personale nel deposito).
Licenza: titolo e abstract sono metadati arXiv distribuiti in CC0 1.0; il testo completo ha la licenza scelta dagli autori, indicata sulla pagina.
Letto il 2026-11-03T11:12:52.623Z dalla pagina https://arxiv.org/list/gr-qc/new (consentita dal robots.txt di arxiv.org, con il suo crawl-delay).