Zobrazeno 1 - 10
of 44
pro vyhledávání: '"Keigo Fukumura"'
Autor:
Oluwashina K. Adegoke, Javier A. García, Riley M. T. Connors, Yuanze Ding, Guglielmo Mastroserio, James F. Steiner, Adam Ingram, Fiona A. Harrison, John A. Tomsick, Erin Kara, Missagh Mehdipour, Keigo Fukumura, Daniel Stern, Santiago Ubach, Matteo Lucchini
Publikováno v:
The Astrophysical Journal, Vol 977, Iss 1, p 26 (2024)
MAXI J1803-298 is a transient black hole candidate discovered in 2021 May during an outburst that lasted several months. Multiple X-ray observations reveal recurring “dipping” intervals in several of its light curves, particularly during the hard
Externí odkaz:
https://doaj.org/article/3c6e2d7943214ab0a144d8d7440a3aa1
Autor:
Keigo Fukumura, Missagh Mehdipour, Ehud Behar, Chris Shrader, Mauro Dadina, Demosthenes Kazanas, Stefano Marchesi, Francesco Tombesi
Publikováno v:
The Astrophysical Journal, Vol 968, Iss 2, p 70 (2024)
X-ray obscuration of active galactic nuclei (AGNs) is considered in the context of ionized winds of stratified structure launched from accretion disks. We argue that a Compton-thick layer of a large-scale disk wind can obscure continuum X-rays and al
Externí odkaz:
https://doaj.org/article/3c7689ffba374144888d5d2d687e361a
Autor:
Keigo Fukumura, Mauro Dadina, Gabriele Matzeu, Francesco Tombesi, Chris Shrader, Demosthenes Kazanas
We aim to explore spectral signatures of the predicted multi-ion UFOs in the broadband X-ray spectra of active galactic nuclei (AGNs) by exploiting an accretion disk wind model in the context of a simple magnetohydrodynamic (MHD) framework. We are fo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5aa130b66a12469acefa522b47e8af63
http://arxiv.org/abs/2205.08894
http://arxiv.org/abs/2205.08894
Autor:
Abraham J. Reines, Keigo Fukumura
Publikováno v:
Research Notes of the AAS. 6:243
We investigate hard X-ray obscuration of Active Galactic Nuclei (AGNs) by considering photoionization processes for a number of simulated accretion-disk winds in our magnetohydrodynamic (MHD) framework. To follow up our earlier work on calculating sy
Autor:
Francesco Tombesi, John A. Tomsick, Sudip Bhattacharyya, Sudip Chakraborty, Ajay Ratheesh, Gaurava K. Jaisawal, Keigo Fukumura
Publikováno v:
Chakraborty, S, Ratheesh, A, Bhattacharyya, S, Tomsick, J A, Tombesi, F, Fukumura, K & Jaisawal, G K 2021, ' NuSTAR monitoring of MAXI J1348−630: evidence of high density disc reflection ', Monthly Notices of the Royal Astronomical Society, vol. 508, no. 1, pp. 475-488 . https://doi.org/10.1093/mnras/stab2530
We present the broadband spectral analysis of all the six hard, intermediate and soft state NuSTAR observations of the recently discovered transient black hole X-ray binary MAXI J1348-630 during its first outburst in 2019. We first model the data wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::44e034d7fd4ac23bb9ae208ae0bdff3e
https://orbit.dtu.dk/en/publications/e6c962a4-2adb-438f-9caf-c3b670de5211
https://orbit.dtu.dk/en/publications/e6c962a4-2adb-438f-9caf-c3b670de5211
Autor:
Constantinos Kalapotharakos, Demosthenes Kazanas, Chris Shrader, Francesco Tombesi, Keigo Fukumura, Ehud Behar
We analyze three prototypical black hole (BH) X-ray binaries (XRBs), \4u1630, \gro1655\ and \h1743, in an effort to systematically understand the intrinsic state transition of the observed accretion-disk winds between \windon\ and \windoff\ states by
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::52476a417685f8b3fb1c604e6cbec273
Autor:
Abraham J. Reines, Keigo Fukumura
Publikováno v:
Research Notes of the AAS. 6:123
We investigate obscuration of Active Galactic Nuclei (AGNs), identified as Supermassive Black Holes (BH) in luminous galaxies. In this model, winds of plasma particles launched from the accretion disk are photoionized by hard X-ray continua from the
Autor:
Cory Jones, Keigo Fukumura
Publikováno v:
Research Notes of the AAS. 6:118
High energy coronal radiation in Black Hole X-Ray Binary sources is often absorbed by accretion disk winds and the resulting absorption signatures heavily depend on its ionizing spectral energy distribution (SED). Considering multiple ion absorbers i
Publikováno v:
Mon Not R Astron Soc Lett
Observations of X-ray absorption lines in magnetically driven disk winds around black hole binaries and active galactic nuclei yield a universal radial density profile rho proportional to r^{-1.2} in the wind. This is in disagreement with the standar
Autor:
Keigo Fukumura, Kaitlyn Porter
We consider a temporal response of relativistically broadened line spectrum of iron from black hole accretion irradiated by an X-ray echo under strong gravity. The physical condition of accreting gas is numerically calculated in the context of genera
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::80c787d8ae1362d196a85fb77732cede
http://arxiv.org/abs/2002.09550
http://arxiv.org/abs/2002.09550