Zobrazeno 1 - 10
of 29
pro vyhledávání: '"I. Psaradaki"'
Autor:
P. Kosec, D. Rogantini, E. Kara, C. R. Canizares, A. C. Fabian, C. Pinto, I. Psaradaki, R. Staubert, D. J. Walton
Publikováno v:
The Astrophysical Journal, Vol 972, Iss 1, p 32 (2024)
X-ray binaries are known to launch powerful accretion disk winds that can have a significant impact on the binary systems and their surroundings. To quantify the impact and determine the launching mechanisms of these outflows, we need to measure the
Externí odkaz:
https://doaj.org/article/17a1c526fe434bedaaa8fc7402f5dbf7
Autor:
I. Psaradaki, L. Corrales, J. Werk, A. G. Jensen, E. Costantini, M. Mehdipour, R. Cilley, N. Schulz, J. Kaastra, J. A. García, L. Valencic, T. Kallman, F. Paerels
Publikováno v:
The Astronomical Journal, Vol 167, Iss 5, p 217 (2024)
In this study, we investigate interstellar absorption lines along the line of sight toward the galactic low-mass X-ray binary Cygnus X-2. We combine absorption line data obtained from high-resolution X-ray spectra collected with the Chandra and XMM-N
Externí odkaz:
https://doaj.org/article/eb6e73043c5e459d9c57aa12679a5868
Autor:
P. Kosec, E. Kara, A. C. Fabian, C. Pinto, I. Psaradaki, D. Rogantini, R. Staubert, D. J. Walton
Publikováno v:
The Astrophysical Journal, Vol 959, Iss 1, p 51 (2023)
Hercules X-1 is a nearly edge-on X-ray binary with a warped, precessing accretion disk, which manifests through a 35-day cycle of alternating High and Low flux states. This disk precession introduces a changing line of sight toward the X-ray source,
Externí odkaz:
https://doaj.org/article/9edefa409e474408afb665b73c45c750
Autor:
P. Kosec, E. Kara, A. C. Fabian, F. Fürst, C. Pinto, I. Psaradaki, C. S. Reynolds, D. Rogantini, D. J. Walton, R. Ballhausen, C. Canizares, S. Dyda, R. Staubert, J. Wilms
The accretion of matter onto black holes and neutron stars often leads to the launching of outflows that can greatly affect the environments surrounding the compact object. In supermassive black holes, these outflows can even be powerful enough to di
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::16f3b69ee50746aa3858cea2d5fa5a10
http://arxiv.org/abs/2304.05490
http://arxiv.org/abs/2304.05490
Akademický článek
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Autor:
I. Psaradaki, E. Costantini, D. Rogantini, M. Mehdipour, L. Corrales, S. T. Zeegers, F. de Groot, J. W. A. den Herder, H. Mutschke, S. Trasobares, C. P. de Vries, L. B. F. M. Waters
Publikováno v:
Astronomy & Astrophysics, 670, 1-12
Astronomy & Astrophysics, 670, pp. 1-12
Astronomy & Astrophysics, 670, pp. 1-12
Understanding the chemistry of the interstellar medium (ISM) is fundamental for the comprehension of the Galactic and stellar evolution. X-rays provide an excellent way to study the dust chemical composition and crystallinity along different sight-li
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e204c406b7f024ca8112ea3e3b48a7f
https://doi.org/10.1051/0004-6361/202244110
https://doi.org/10.1051/0004-6361/202244110
Autor:
I. Psaradaki, Jon M. Miller, Nathalie Degenaar, Aastha S. Parikh, David Modiano, J. V. Hernández Santisteban, Rudy Wijnands, Elisa Costantini
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 501(1), 1453-1462. Oxford University Press
The accretion behaviour in low-mass X-ray binaries (LMXBs) at low luminosities, especially at 3500 km/s), which could indicate that it results from an outflow such as a pulsar wind. By studying several epochs of X-ray and near-UV data obtained with X
Autor:
P. Kosec, E. Kara, A. C. Fabian, F. Fürst, C. Pinto, I. Psaradaki, C. S. Reynolds, D. Rogantini, D. J. Walton, R. Ballhausen, C. Canizares, S. Dyda, R. Staubert, J. Wilms
Publikováno v:
The Astrophysical Journal. 936:185
Hercules X-1 is a nearly edge-on accreting X-ray pulsar with a warped accretion disk, precessing with a period of about 35 days. The disk precession allows for unique and changing sightlines towards the X-ray source. To investigate the accretion flow
Akademický článek
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Akademický článek
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