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Kawanaka, Norita, Kato, Yoshiaki, Mineshige, Shin (2008) X-Ray Emissions from Three-Dimensional Magnetohydrodynamic Coronal Accretion Flows. Publications of the Astronomical Society of Japan, 60 (2). 399-405 doi:10.1093/pasj/60.2.399

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Reference TypeJournal (article/letter/editorial)
TitleX-Ray Emissions from Three-Dimensional Magnetohydrodynamic Coronal Accretion Flows
JournalPublications of the Astronomical Society of Japan
AuthorsKawanaka, NoritaAuthor
Kato, YoshiakiAuthor
Mineshige, ShinAuthor
Year2008 (April 25)Volume60
Issue2
PublisherOxford University Press (OUP)
DOIdoi:10.1093/pasj/60.2.399Search in ResearchGate
Generate Citation Formats
Mindat Ref. ID3598321Long-form Identifiermindat:1:5:3598321:3
GUID0
Full ReferenceKawanaka, Norita, Kato, Yoshiaki, Mineshige, Shin (2008) X-Ray Emissions from Three-Dimensional Magnetohydrodynamic Coronal Accretion Flows. Publications of the Astronomical Society of Japan, 60 (2). 399-405 doi:10.1093/pasj/60.2.399
Plain TextKawanaka, Norita, Kato, Yoshiaki, Mineshige, Shin (2008) X-Ray Emissions from Three-Dimensional Magnetohydrodynamic Coronal Accretion Flows. Publications of the Astronomical Society of Japan, 60 (2). 399-405 doi:10.1093/pasj/60.2.399
In(2008, April) Publications of the Astronomical Society of Japan Vol. 60 (2) Oxford University Press (OUP)

See Also

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Ohsuga, Ken, Mineshige, Shin, Mori, Masao, Kato, Yoshiaki (2009) Global Radiation-Magnetohydrodynamic Simulations of Black-Hole Accretion Flow and Outflow: Unified Model of Three States. Publications of the Astronomical Society of Japan, 61 (3). doi:10.1093/pasj/61.3.l7
Kawanaka, Norita, Mineshige, Shin (2024) Model of a “Warm Corona” as the origin of the soft X-ray excess of active galactic nuclei. Publications of the Astronomical Society of Japan, 76 (2) 306-315 doi:10.1093/pasj/psae012
Kawanaka, Norita, Mineshige, Shin (2021) What determines the unique spectra of super-Eddington accretors? Origin of optically thick and low-temperature coronae in super-Eddington accretion flows. Publications of the Astronomical Society of Japan, 73 (3) 630-638 doi:10.1093/pasj/psab023
Kato, Yoshiaki (2004) 2:3 Twin Quasi-Periodic Oscillations in Magnetohydrodynamic Accretion Flows. Publications of the Astronomical Society of Japan, 56 (5). 931-937 doi:10.1093/pasj/56.5.931
Ohsuga, Ken, Kato, Yoshiaki, Mineshige, Shin (2005) Spectral Properties of Three‐dimensional Magnetohydrodynamic Accretion Flows. The Astrophysical Journal, 627 (2). 782-789 doi:10.1086/430432
Kimura, Mariko, Mineshige, Shin, Kawanaka, Norita (2015) How does a secular instability grow in a hyperaccretion flow?. Publications of the Astronomical Society of Japan, 67 (5). 101pp. doi:10.1093/pasj/psv070
Mizumoto, Misaki, Moriyama, Kotaro, Ebisawa, Ken, Mineshige, Shin, Kawanaka, Norita, Tsujimoto, Masahiro (2018) Can the relativistic light-bending model explain X-ray spectral variations of Seyfert galaxies?. Publications of the Astronomical Society of Japan, 70 (3). doi:10.1093/pasj/psy032
Kawabata, Ryoji, Mineshige, Shin (2009) Thermally Driven Winds from Radiatively Inefficient Accretion Flows. Publications of the Astronomical Society of Japan, 61 (5). 1135-1141 doi:10.1093/pasj/61.5.1135
Vierdayanti, Kiki, Watarai, Ken-ya, Mineshige, Shin (2008) On Black Hole Mass Estimation from X-Ray Spectra of Ultraluminous X-Ray Sources. Publications of the Astronomical Society of Japan, 60 (3). 653-665 doi:10.1093/pasj/60.3.653
Hayasaki, Kimitake, Saito, Hideki, Mineshige, Shin (2013) Binary Black Hole Accretion Flows From a Misaligned Circumbinary Disk. Publications of the Astronomical Society of Japan, 65 (4). 86pp. doi:10.1093/pasj/65.4.86
Hayasaki, Kimitake, Mineshige, Shin, Sudou, Hiroshi (2007) Binary Black Hole Accretion Flows in Merged Galactic Nuclei. Publications of the Astronomical Society of Japan, 59 (2). 427-441 doi:10.1093/pasj/59.2.427
 
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