Zobrazeno 1 - 10
of 12
pro vyhledávání: '"R M T Connors"'
Autor:
L Mallick, A C Fabian, J A García, J A Tomsick, M L Parker, T Dauser, D R Wilkins, B De Marco, J F Steiner, R M T Connors, G Mastroserio, A G Markowitz, C Pinto, W N Alston, A M Lohfink, P Gandhi
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 513:4361-4379
The standard alpha-disc model predicts an anti-correlation between the density of the inner accretion disc and the black hole mass times square of the accretion rate, as seen in higher mass ($M_{\rm BH}>10^{6} M_{\odot}$) active galactic nuclei (AGNs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f81b82f5cb6d7bec277778b37b5fbbf0
https://doi.org/10.1093/mnras/stac990
https://doi.org/10.1093/mnras/stac990
Autor:
G. Mastroserio, B. W. Grefenstette, P. Thalhammer, D. J. K. Buisson, M. C. Brumback, R. M. Ludlam, R. M. T. Connors, J. A. García, V. Grinberg, K. K. Madsen, H. Miyasaka, J. A. Tomsick, J. Wilms
Due to the structure of the NuSTAR telescope, photons at large off-axis (> 1deg) can reach the detectors directly (stray light), without passing through the instrument optics. At these off-axis angles NuSTAR essentially turns into a collimated instru
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::80b6f8a6e3fe6f5a7880b314362612de
https://opus4.kobv.de/opus4-fau/frontdoor/index/index/docId/21133
https://opus4.kobv.de/opus4-fau/frontdoor/index/index/docId/21133
Autor:
M Lucchini, C Ceccobello, S Markoff, Y Kini, A Chhotray, R M T Connors, P Crumley, H Falcke, D Kantzas, D Maitra
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 517(4), 5853-5881. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 517, 5853-5881
Monthly Notices of the Royal Astronomical Society, 517, 4, pp. 5853-5881
Monthly Notices of the Royal Astronomical Society, 517, 5853-5881
Monthly Notices of the Royal Astronomical Society, 517, 4, pp. 5853-5881
Accreting black holes are sources of major interest in astronomy, particular those launching jets because of their ability to accelerate particles, and dramatically affect their surrounding environment up to very large distances. The spatial, energy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b74d6084256fbb620b0daa2ee38e4f91
https://dare.uva.nl/personal/pure/en/publications/bhjet-a-public-multizone-steady-state-jet--thermal-corona-spectral-model(e1059ad6-cfe6-454b-a1b4-5b5debca0fd8).html
https://dare.uva.nl/personal/pure/en/publications/bhjet-a-public-multizone-steady-state-jet--thermal-corona-spectral-model(e1059ad6-cfe6-454b-a1b4-5b5debca0fd8).html
Autor:
Ole König, Adam Ingram, Jingyi Wang, Fiona A. Harrison, Matteo Lucchini, Erin Kara, R. M. T. Connors, Yuri Cavecchi, Javier A. García, Thomas Dauser, Michiel van der Klis, Guglielmo Mastroserio
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 507(1), 55-73. Oxford University Press
We present a new release of the RELTRANS model to fit the complex cross-spectrum of accreting black holes as a function of energy. The model accounts for continuum lags and reverberation lags self-consistently in order to consider the widest possible
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b810a1046597354291af02122265f623
https://doi.org/10.1093/mnras/stab2056
https://doi.org/10.1093/mnras/stab2056
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 510(4), 5187-5198. Oxford University Press
Since the discovery of cosmic rays (CRs) over a century ago, their origin remains an open question. Galactic CRs with energy up to the knee ($10^{15}$ eV) are considered to originate from supernova remnants, but this scenario has recently been questi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7f3d766f0694473339f7c3d60b24ebd
https://resolver.caltech.edu/CaltechAUTHORS:20220329-55502504
https://resolver.caltech.edu/CaltechAUTHORS:20220329-55502504
We study the effect of returning radiation on the shape of the X-ray reflection spectrum in the case of thin accretion disks. We show that the returning radiation mainly influences the observed reflection spectrum for a large black hole spin (a > 0.9
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f42af31a1ed7fab0ef993634c292b5c
Autor:
Sera Markoff, Lucy Heil, Chiara Ceccobello, D. Kantzas, R. M. T. Connors, Marco Toliman Lucchini, D. van Eijnatten, Victoria Grinberg, P. Crumley
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 485(3), 3696-3714. Oxford University Press
GX~339$-$4 is a black hole X-ray binary that is a key focus of accretion studies since it goes into outburst roughly every two-to-three years. Tracking of its radio, IR and X-ray flux during multiple outbursts reveals tight broadband correlations. Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6101ea944140adea82e15b2982bd6ce0
https://doi.org/10.1093/mnras/stz604
https://doi.org/10.1093/mnras/stz604
Autor:
Francesca Scarcella, Massimo Ricotti, Daniele Gaggero, Gianfranco Bertone, Julien Manshanden, R. M. T. Connors
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 505(3), 4036-4047. Oxford University Press
Isolated black holes in our Galaxy have eluded detection so far. We present here a comprehensive study on the detectability of isolated stellar-mass astrophysical black holes that accrete interstellar gas from molecular clouds in both the local regio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f2ba18dc003689f793589a4205830864
http://arxiv.org/abs/2012.10421
http://arxiv.org/abs/2012.10421
Autor:
Victoria Grinberg, Javier A. García, John A. Tomsick, Joern Wilms, R. M. T. Connors, Fiona A. Harrison, Stefan Licklederer, Navin Sridhar, James F. Steiner, Thomas Dauser
We explore the accretion properties of the black hole X-ray binary \j1550\ during its outbursts in 1998/99 and 2000. We model the disk, corona, and reflection components of X-ray spectra taken with the {\it Rossi X-ray Timing Explorer} (\rxte), using
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3e1990c9a5571e43d15fd148d0e9f36b
http://arxiv.org/abs/2002.11873
http://arxiv.org/abs/2002.11873
Autor:
Amanda Weltman, Mairi Sakellariadou, Francesca Vidotto, Laura Wolz, M. Méndez-Isla, Hamsa Padmanabhan, Ian Harrison, Jose A. R. Cembranos, Roy Maartens, Philip Bull, R. M. T. Connors, Alkistis Pourtsidou, Chris Clarkson, Peter K. S. Dunsby, A. de la Cruz-Dombriz, Céline Bœhm, Christoph Weniger, Tejaswi Venumadhav, T. Trombetti, Stefano Camera, Katharine Kelley, Signe Riemer-Sørensen, Gianfranco Bertone, J. Silk, Bryan Gaensler, Carlo Burigana, Marcus Brüggen, Julien Larena, Peter J. Quinn, Franco Vazza, Francisco Villaescusa-Navarro, Camille Bonvin, Martin Sahlén, Lijing Shao, Daniele Gaggero, Rennan Barkana, Albert Bosma, Soumya D. Mohanty, Yin-Zhe Ma, Sambatra Andrianomena, Nicolao Fornengo, Alvise Raccanelli, E. Athanassoula, Steven G. Murray, Yue-Fei Wang, José Fonseca, Jonathan R. Pritchard, Fupeng Zhang, David Parkinson, David Bacon, Francesca Calore, Marco Regis, Prasenjit Saha
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
Publ.Astron.Soc.Austral.
Publ.Astron.Soc.Austral., 2020, 37, pp.e002. ⟨10.1017/pasa.2019.42⟩
Publications of the Astronomical Society of Australia
Weltman, A, Bull, P, Camera, S, Kelley, K, Padmanabhan, H, Pritchard, J, Raccanelli, A, Riemer-Sørensen, S, Shao, L, Andrianomena, S, Athanassoula, E, Bacon, D, Barkana, R, Bertone, G, Bœhm, C, Bonvin, C, Bosma, A, Brüggen, M, Burigana, C, Calore, F, Cembranos, J A R, Clarkson, C, Connors, R M T, Cruz-Dombriz, D L, Dunsby, P K S, Fonseca, J, Fornengo, N, Gaggero, D, Harrison, I, Larena, J, Ma, Y Z, Maartens, R, Méndez-Isla, M, Mohanty, S D, Murray, S, Parkinson, D, Pourtsidou, A, Quinn, P J, Regis, M, Saha, P, Sahlén, M, Sakellariadou, M, Silk, J, Trombetti, T, Vazza, F, Venumadhav, T, Vidotto, F, Villaescusa-Navarro, F, Wang, Y, Weniger, C, Wolz, L, Zhang, F & Gaensler, B M 2020, ' Fundamental physics with the Square Kilometre Array ', Publications of the Astronomical Society of Australia, vol. 37, e002 . https://doi.org/10.1017/pasa.2019.42
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
instname
E-Prints Complutense. Archivo Institucional de la UCM
Publ.Astron.Soc.Austral.
Publ.Astron.Soc.Austral., 2020, 37, pp.e002. ⟨10.1017/pasa.2019.42⟩
Publications of the Astronomical Society of Australia
Weltman, A, Bull, P, Camera, S, Kelley, K, Padmanabhan, H, Pritchard, J, Raccanelli, A, Riemer-Sørensen, S, Shao, L, Andrianomena, S, Athanassoula, E, Bacon, D, Barkana, R, Bertone, G, Bœhm, C, Bonvin, C, Bosma, A, Brüggen, M, Burigana, C, Calore, F, Cembranos, J A R, Clarkson, C, Connors, R M T, Cruz-Dombriz, D L, Dunsby, P K S, Fonseca, J, Fornengo, N, Gaggero, D, Harrison, I, Larena, J, Ma, Y Z, Maartens, R, Méndez-Isla, M, Mohanty, S D, Murray, S, Parkinson, D, Pourtsidou, A, Quinn, P J, Regis, M, Saha, P, Sahlén, M, Sakellariadou, M, Silk, J, Trombetti, T, Vazza, F, Venumadhav, T, Vidotto, F, Villaescusa-Navarro, F, Wang, Y, Weniger, C, Wolz, L, Zhang, F & Gaensler, B M 2020, ' Fundamental physics with the Square Kilometre Array ', Publications of the Astronomical Society of Australia, vol. 37, e002 . https://doi.org/10.1017/pasa.2019.42
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Square Kilometre Array: et al.
arXiv:1810.02680v3
The Square Kilometre Array (SKA) is a planned large radio interferometer designed to operate over a wide range of frequencies, and with an order of magnitude greater sensitivity and survey s
arXiv:1810.02680v3
The Square Kilometre Array (SKA) is a planned large radio interferometer designed to operate over a wide range of frequencies, and with an order of magnitude greater sensitivity and survey s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79b574df1e370cf93bfe355d9902f579
http://hdl.handle.net/10261/236902
http://hdl.handle.net/10261/236902