Zobrazeno 1 - 10
of 81
pro vyhledávání: '"Jeroen Homan"'
Autor:
Edward Nathan, Adam Ingram, Jeroen Homan, Daniela Huppenkothen, Phil Uttley, Michiel van der Klis, Sara Motta, Diego Altamirano, Matthew Middleton
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 511(1), 255-279. Oxford University Press
Quasi-periodic oscillations (QPOs) are often present in the X-ray flux from accreting stellar-mass black holes (BHs). If they are due to relativistic (Lense-Thirring) precession of an inner accretion flow which is misaligned with the disc, the iron e
Autor:
Dany Page, Jeroen Homan, Martin Nava-Callejas, Yuri Cavecchi, Mikhail V. Beznogov, Nathalie Degenaar, Rudy Wijnands, Aastha S. Parikh
Publikováno v:
Astrophysical Journal, 933(2):933. IOP Publishing Ltd.
The study of transiently accreting neutron stars provides a powerful means to elucidate the properties of neutron star crusts. We present extensive numerical simulations of the evolution of the neutron star in the transient low-mass X-ray binary MAXI
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d81c808d10792770bb795b399774daa9
https://dare.uva.nl/personal/pure/en/publications/a-hyperburst-in-the-maxi-j0556332-neutron-star(80cd24de-591b-4bb5-bb0c-f62c116a9dcd).html
https://dare.uva.nl/personal/pure/en/publications/a-hyperburst-in-the-maxi-j0556332-neutron-star(80cd24de-591b-4bb5-bb0c-f62c116a9dcd).html
Autor:
N. Castro Segura, Francesco Tombesi, Tod E. Strohmayer, Zaven Arzoumanian, Jon M. Miller, Keith C. Gendreau, A. C. Albayati, D. J. K. Buisson, Deepto Chakrabarty, Poshak Gandhi, Dom Walton, Tolga Guver, Diego Altamirano, Sebastien Guillot, John A. Tomsick, C. Malacaria, F. M. Vincentelli, Ron Remillard, Jeroen Homan, Jeremy Hare, Jiachen Jiang, Gaurava K. Jaisawal, M. Ozbey Arabaci, Peter Bult, G. C. Mancuso
Publikováno v:
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 499 (1), pp.793-803. ⟨10.1093/mnras/staa2749⟩
Buisson, D J K, Altamirano, D, Bult, P, Mancuso, G C, Güver, T, Jaisawal, G K, Hare, J, Albayati, A C, Arzoumanian, Z, Segura, N C, Chakrabarty, D, Gandhi, P, Guillot, S, Homan, J, Gendreau, K C, Jiang, J, Malacaria, C, Miller, J M, Arabacı, M Ö, Remillard, R, Strohmayer, T E, Tombesi, F, Tomsick, J A, Vincentelli, F M & Walton, D J 2020, ' Discovery of thermonuclear (Type I) X-ray bursts in the X-ray binary Swift J1858.6–0814 observed with NICER and NuSTAR ', Monthly Notices of the Royal Astronomical Society, vol. 499, pp. 793-803 . https://doi.org/10.1093/mnras/staa2749
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Universidad Nacional de La Plata
instacron:UNLP
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2020, 499 (1), pp.793-803. ⟨10.1093/mnras/staa2749⟩
Buisson, D J K, Altamirano, D, Bult, P, Mancuso, G C, Güver, T, Jaisawal, G K, Hare, J, Albayati, A C, Arzoumanian, Z, Segura, N C, Chakrabarty, D, Gandhi, P, Guillot, S, Homan, J, Gendreau, K C, Jiang, J, Malacaria, C, Miller, J M, Arabacı, M Ö, Remillard, R, Strohmayer, T E, Tombesi, F, Tomsick, J A, Vincentelli, F M & Walton, D J 2020, ' Discovery of thermonuclear (Type I) X-ray bursts in the X-ray binary Swift J1858.6–0814 observed with NICER and NuSTAR ', Monthly Notices of the Royal Astronomical Society, vol. 499, pp. 793-803 . https://doi.org/10.1093/mnras/staa2749
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Swift J1858.6-0814 is a recently discovered X-ray binary notable for extremely strong variability (by factors $>100$ in soft X-rays) in its discovery state. We present the detection of five thermonuclear (Type I) X-ray bursts from Swift J1858.6-0814,
Autor:
Francesco Tombesi, Zaven Arzoumanian, James F. Steiner, Jeroen Homan, M. Ng, Edward M. Cackett, Tod E. Strohmayer, Ronald A. Remillard, Diego Altamirano, Keith C. Gendreau, William Alston, Dheeraj R. Pasham, Deepto Chakrabarty, Jon M. Miller, Peter Bult, Alice K. Harding, Andrew C. Fabian, Brian Metzger, Wynn C. G. Ho
The brightest Fast Blue Optical Transients (FBOTs) are mysterious extragalactic explosions that may represent a new class of astrophysical phenomena. Their fast time to maximum brightness of less than a week and decline over several months and atypic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::83f0daf043589a1588744beaae8cfc70
http://hdl.handle.net/2108/300699
http://hdl.handle.net/2108/300699
Autor:
Jeroen Homan, Keith C. Gendreau, Diego Altamirano, Zaven Arzoumanian, Christian Malacaria, Jon M. Miller, Michael Parker, Gaurava K. Jaisawal, Jérôme Chenevez, David R. Ballantyne, Peter Bult, Tod E. Strohmayer, Andrew C. Fabian
Publikováno v:
Bult, P, Altamirano, D, Arzoumanian, Z, Ballantyne, D R, Chenevez, J, Fabian, A C, Gendreau, K C, Homan, J, Jaisawal, G K, Malacaria, C, Miller, J M, Parker, M L & Strohmayer, T E 2021, ' On the Impact of an Intermediate Duration X-Ray Burst on the Accretion Environment in IGR J17062-6143 ', Astrophysical Journal Supplement Series, vol. 920, no. 1, 59 . https://doi.org/10.3847/1538-4357/ac18c4
We report on a spectroscopic analysis of the X-ray emission from IGR J17062-6143 in the aftermath of its June 2020 intermediate duration Type I X-ray burst. Using the Neutron Star Interior Composition Explorer, we started observing the source three h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e470a31e989c7b04b1dededd85719ee5
http://arxiv.org/abs/2107.13543
http://arxiv.org/abs/2107.13543
Autor:
K. Alabarta, Jeroen Homan, D. J. K. Buisson, J. Neilsen, Arkadip Basak, Tod E. Strohmayer, Zaven Arzoumanian, Keith C. Gendreau, R. Remillard, James F. Steiner, Mariano Mendez, Federico García, Liang Zhang, Diego Altamirano, C. B. Markwardt, P. Uttley
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 505(3), 3823-3843. Oxford University Press
We present a systematic spectral-timing analysis of a fast appearance/disappearance of a type-B quasi-periodic oscillation (QPO), observed in four NICER observations of MAXI J1348-630. By comparing the spectra of the period with and without the type-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8650eb84262edf3bad8d3e5dd280d99
http://arxiv.org/abs/2105.12338
http://arxiv.org/abs/2105.12338
Autor:
Edward M. Cackett, Nathalie Degenaar, Craig O. Heinke, Jeroen Homan, L. E. Rivera Sandoval, Diego Altamirano, G. R. Sivakoff, Jon M. Miller, Arash Bahramian, Rudy Wijnands, Aastha S. Parikh, Yuri Cavecchi
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 479(2), 2777-2788. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 479(2), 2777-2788. Oxford University Press
EXO 1745-248 is a transient neutron-star low-mass X-ray binary that resides in the globular cluster Terzan 5. We studied the transient during its quiescent state using 18 Chandra observations of the cluster acquired between 2003 and 2016. We found an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::53254b7f68890c03ae3bb36e1cff808d
https://dare.uva.nl/personal/pure/en/publications/extreme-quiescent-variability-of-the-transient-neutron-star-lowmass-xray-binary-exo-1745248-in-terzan-5(3797e3b1-be78-4ccd-a1b7-85f10d689a91).html
https://dare.uva.nl/personal/pure/en/publications/extreme-quiescent-variability-of-the-transient-neutron-star-lowmass-xray-binary-exo-1745248-in-terzan-5(3797e3b1-be78-4ccd-a1b7-85f10d689a91).html
Autor:
Ronald A. Remillard, Aaron J. Romanowsky, Natalie A. Webb, Jay Strader, Dacheng Lin, Didier Barret, Olivier Godet, Jeroen Homan, Jimmy A. Irwin
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2020, 892 (2), pp.L25. ⟨10.3847/2041-8213/ab745b⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2020, 892 (2), pp.L25. ⟨10.3847/2041-8213/ab745b⟩
We recently discovered the X-ray/optical outbursting source 3XMM J215022.4-055108. It was best explained as the tidal disruption of a star by an intermediate-mass black hole of mass of a few tens of thousand solar masses in a massive star cluster at
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0748120d47330d3eb32d019b3d1e3943
https://hal.archives-ouvertes.fr/hal-02497819
https://hal.archives-ouvertes.fr/hal-02497819
Autor:
Robert Beswick, Elmar Körding, Assaf Horesh, Rob Fender, David Titterington, Sara Motta, Patrick A. Woudt, David A. H. Buckley, Stephane Corbel, David A. Green, Joe Bright, Elena Gallo, J. Moldon, Antonia Rowlinson, Ian Heywood, R. P. Armstrong, Ralph A. M. J. Wijers, Evangelia Tremou, A. J. van der Horst, Gregory R. Sivakoff, Vanessa McBride, James Miller-Jones, David R. Williams, Thomas D. Russell, Richard M. Plotkin, Alexandra J. Tetarenko, Paul J. Groot, Jeroen Homan
Publikováno v:
Nature Astron.
Nature Astron., 2020, 4 (7), pp.697-703. ⟨10.1038/s41550-020-1023-5⟩
Nature Astron., 2020, 4 (7), pp.697-+. ⟨10.1038/s41550-020-1023-5⟩
Nature Astronomy, 4, 697-703
Nature Astronomy, 697-703. Nature Publishing Group
STARTPAGE=697;ENDPAGE=703;ISSN=2397-3366;TITLE=Nature Astronomy
Digital.CSIC. Repositorio Institucional del CSIC
instname
Nature Astronomy, 4, 7, pp. 697-703
Nature Astron., 2020, 4 (7), pp.697-703. ⟨10.1038/s41550-020-1023-5⟩
Nature Astron., 2020, 4 (7), pp.697-+. ⟨10.1038/s41550-020-1023-5⟩
Nature Astronomy, 4, 697-703
Nature Astronomy, 697-703. Nature Publishing Group
STARTPAGE=697;ENDPAGE=703;ISSN=2397-3366;TITLE=Nature Astronomy
Digital.CSIC. Repositorio Institucional del CSIC
instname
Nature Astronomy, 4, 7, pp. 697-703
Black holes in binary systems execute patterns of outburst activity where two characteristic X-ray states are associated with different behaviours observed at radio wavelengths. The hard state is associated with radio emission indicative of a continu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64ce504df40046a24d91b7e62601cd02
https://hal.archives-ouvertes.fr/hal-02518057/document
https://hal.archives-ouvertes.fr/hal-02518057/document
Autor:
Rudy Wijnands, J. J. M. in 't Zand, Jeroen Homan, D. M. Russell, D. A. H. Buckley, E. J. Kotze, Aastha S. Parikh, A. J. Goodwin, D. de Martino, D. M. Bramich, Duncan K. Galloway, Alessandro Papitto, Fraser Lewis, Maria Cristina Baglio, Craig O. Heinke
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 498(3), 3429-3439. Oxford University Press
X-ray transients, such as accreting neutron stars, periodically undergo outbursts, thought to be caused by a thermal-viscous instability in the accretion disk. Usually outbursts of accreting neutron stars are identified when the accretion disk has un
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dd5916624e2a968c7ec3e479bcdfceb0
http://hdl.handle.net/20.500.12386/31275
http://hdl.handle.net/20.500.12386/31275