Zobrazeno 1 - 10
of 10
pro vyhledávání: '"M. J. P. Wijngaarden"'
Autor:
Rudy Wijnands, Mikhail V. Beznogov, L. S. Ootes, Nathalie Degenaar, Philip Chang, M. J. P. Wijngaarden, Dany Page, Wynn C. G. Ho, Andrew Cumming
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 493(4), 4936-4944. Oxford University Press
Valuable information about the neutron star interior can be obtained by comparing observations of thermal radiation from a cooling neutron star crust with theoretical models. Nuclear burning of lighter elements that diffuse to deeper layers of the en
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b44ea0dddac4bf0b1c180692831d1726
https://dare.uva.nl/personal/pure/en/publications/the-effect-of-diffusive-nuclear-burning-in-neutron-star-envelopes-on-cooling-in-accreting-systems(610781a3-3bed-4044-a318-c5701e829a03).html
https://dare.uva.nl/personal/pure/en/publications/the-effect-of-diffusive-nuclear-burning-in-neutron-star-envelopes-on-cooling-in-accreting-systems(610781a3-3bed-4044-a318-c5701e829a03).html
Autor:
M. J. P. Wijngaarden, Yue Zhao, Craig O. Heinke, P. S. Shternin, Wynn C. G. Ho, David L. Kaplan
We present analysis of multiple Chandra and XMM-Newton spectra, separated by 9-19 years, of four of the youngest central compact objects (CCOs) with ages < 2500 yr: CXOU J232327.9+584842 (Cassiopeia A), CXOU J160103.1-513353 (G330.2+1.0), 1WGA J1713.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd5eae466028d04eb0a13c7980fbd847
https://eprints.soton.ac.uk/452609/
https://eprints.soton.ac.uk/452609/
Autor:
M. J. P. Wijngaarden, P. S. Shternin, D. D. Ofengeim, Wynn C. G. Ho, Daniel J. Patnaude, Craig O. Heinke
We present a new model-independent (applicable for a broad range of equations of state) analysis of the neutrino emissivity due to triplet neutron pairing in neutron star cores. We find that the integrated neutrino luminosity of the Cooper Pair Forma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1e9a550db385a5a8d96c3e09f5e7c5df
http://arxiv.org/abs/2106.05692
http://arxiv.org/abs/2106.05692
Autor:
M. J. P. Wijngaarden, Dany Page, Craig O. Heinke, Mikhail V. Beznogov, Wynn C. G. Ho, Daniel J. Patnaude, Philip Chang
The study of how neutron stars cool over time can provide invaluable insights into fundamental physics such as the nuclear equation of state and superconductivity and superfluidity. A critical relation in neutron star cooling is the one between obser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7ca2b0d7cb3cef0c5c1ee09b0153fe6d
https://eprints.soton.ac.uk/430315/
https://eprints.soton.ac.uk/430315/
Autor:
Rudy Wijnands, Craig O. Heinke, Dany Page, L. S. Ootes, Nathalie Degenaar, Aastha S. Parikh, Arash Bahramian, Smriti Vats, Edward M. Cackett, M. J. P. Wijngaarden, Jon M. Miller, Jeroen Homan, Diego Altamirano
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 487(1), 1447-1461. Oxford University Press
We present a new Chandra observation (performed in July 2016) of the neutron star X-ray transient IGR J17480-2446, located in the globular cluster Terzan 5. We study the continued cooling of the neutron star crust in this system that was heated durin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::719cc1cbff66b95bef9820b108e500f4
http://arxiv.org/abs/1805.00610
http://arxiv.org/abs/1805.00610
Autor:
Arash Bahramian, Edward F. Brown, Andrew Cumming, L. S. Ootes, Craig O. Heinke, Edward M. Cackett, M. J. P. Wijngaarden, Jeroen Homan, A. Rouco Escorial, Dany Page, Aastha S. Parikh, Rudy Wijnands, Nathalie Degenaar
Publikováno v:
Astronomy & Astrophysics, 624:A84. EDP Sciences
Monitoring the cooling of neutron-star crusts heated during accretion outbursts allows us to infer the physics of the dense matter present in the crust. We examine the crust cooling evolution of the low-mass X-ray binary MXB 1659-29 up to ~505 days a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::13ee42052c0e5e442d0ab0312b105aa5
Publikováno v:
Proceedings of the International Astronomical Union, 13(S337), 229-232. Cambridge University Press
In accreting neutron star X-ray transients, the neutron star crust can be substantially heated out of thermal equilibrium with the core during an accretion outburst. The observed subsequent cooling in quiescence (when accretion has halted) offers a u
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7116e8a61a2722c78135f4261184370b
Autor:
William I. Hartkopf, Matthew W. Muterspaugh, Chris Farrington, Christian A. Hummel, M. J. P. Wijngaarden, Huib F. Henrichs, Gregory W. Henry, Gail Schaefer, R. T. Zavala, Benjamin F. Lane
Publikováno v:
Astronomical Journal, 150(5):140. IOP Publishing Ltd.
The dwarf stars in the 26 year period binary α Com were predicted to eclipse each other in early 2015. That prediction was based on an orbit model made with over 600 astrometric observations using micrometers, speckle interferometry, and long baseli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::45eeea8c76a9799021843781935b8ce5
https://dare.uva.nl/personal/pure/en/publications/predicting-the--comae-berenices-time-of-eclipse-how-3-ambiguous-measurements-out-of-609-caused-a-26-year-binarys-eclipse-to-be-missed(45c00709-e79d-41b2-9d84-bf71d8ca7c35).html
https://dare.uva.nl/personal/pure/en/publications/predicting-the--comae-berenices-time-of-eclipse-how-3-ambiguous-measurements-out-of-609-caused-a-26-year-binarys-eclipse-to-be-missed(45c00709-e79d-41b2-9d84-bf71d8ca7c35).html
Publikováno v:
Ho, W C G, Wijngaarden, M J P, Andersson, N, Tauris, T M & Haberl, F 2020, ' Early neutron star evolution in high-mass X-ray binaries ', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 1, pp. 44-49 . https://doi.org/10.1093/mnras/staa675
The application of standard accretion theory to observations of X-ray binaries provides valuable insights into neutron star properties, such as their spin period and magnetic field. However, most studies concentrate on relatively old systems, where t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::31a4551305e93ce4b642d20f074c35df
Autor:
Matthew W. Muterspaugh, M. J. P. Wijngaarden, H. F. Henrichs, Benjamin F. Lane, William I. Hartkopf, Gregory W. Henry, Gail H. Schaefer, Chris Farrington, Christian A. Hummel, R. T. Zavala
Publikováno v:
Astronomical Journal; Nov2015, Vol. 150 Issue 5, p1-1, 1p