Black hole X-ray binaries: the transition from the cool thin disk to the coronal flow

The corona contracts in a black-hole transient

Kara, E.
Steiner, J. F.
Fabian, A. C.
Cackett, E. M.
Uttley, P.
Remillard, R. A.
Gendreau, K. C.
Arzoumanian, Z.
Altamirano, D.
Eikenberry, S.
Enoto, T.
Homan, J.
Neilsen, J.
Stevens, A. L.

January 2019

The geometry of the accretion flow around stellar-mass black holes can change on timescales of days ...

The formation of the black hole in the X-ray binary system V404 Cyg

Miller-Jones, J.C.A.
Jonker, P.G.
Nelemans, G.A.
Zwart, S. Portegies
Dhawan, V.
Brisken, W.
Gallo, E.
Rupen, M.P.

January 2008

Contains fulltext : 72479.pdf (author's version ) (Open Access)11 p

Tracking the evolution of the accretion flow in MAXI J1820+070 during its hard state with the JED-SAD model

Marino, A.
Barnier, S.
Petrucci, P.O.
del Santo, M.
Malzac, J.
Ferreira, J.
Marcel, G.
Segreto, A.
Motta, S.E.
d'Aì, A.
Di Salvo, T.
Guillot, S.
Russell, T.D.

January 2021

International audienceContext. X-ray binaries in outburst typically show two canonical X-ray spectra...

Black hole X-ray binaries: A new view on soft-hard spectral transitions

Meyer, F.
Meyer-Hofmeister, E. (Max-Planck-Institut fuer Astrophysik, Garching (Germany))
Academia Sinica, Kunming, YN (China). Yunnan Observatory)
Liu, B.F. (Max-Planck-Institut fuer Astrophysik, Garching (Germany)
Max-Planck-Institut fuer Astrophysik, Garching (Germany)

January 2000

SIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB...

Black hole soft X-ray transients: evolution of the cool disk and mass supply for the ADAF

Meyer-Hofmeister, E.
Meyer, F.
Max-Planck-Institut fuer Astrophysik, Garching (Germany)

January 1999

SIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB...

Analytical Model of Disk Evaporation and State Transitions in Accreting Black Holes

Cho, Hyerin
Narayan, Ramesh

June 2022

State transitions in black hole X-ray binaries are likely caused by gas evaporation from a thin accr...

The formation of black hole low-mass X-ray binaries: Through case B or case C mass transfer?

Nelemans, G.A.
Heuvel, E.P.J. van den

January 2001

Contains fulltext : 156202.pdf (preprint version ) (Open Access

Accretion disc coronae in black hole binaries.

Malzac, J.

December 2006

Most of the luminosity of accreting black hole is emitted in the X-ray band. This radiation is belie...

Black hole X-ray transients: mass accumulation in the disk - constraints for the viscosity

Meyer-Hofmeister, E.
Meyer, F.
Max-Planck-Institut fuer Astrophysik, Garching (Germany)

January 2000

The outburst cycles of black hole X-ray transients are now generally understood as caused by a therm...

Accretion disc coronae in black hole binaries

J Malzac

March 2020

Abstract. Most of the luminosity of accreting black hole is emitted in the X-ray band. This radiatio...

The Effect of Coronal Radiation on a Residual Inner Disk in the Low/Hard Spectral State of Black Hole X-ray Binary Systems

Liu, B.F.
Done, C.
Taam, R.E.

January 2011

Thermal conduction between a cool accretion disk and a hot inner corona can result in either evapora...

Wind-type outflows from black hole X-ray binary MAXI J1820+070: the near infrared view

Sánchez-Sierras, Javier
Muñoz-Darias, Teo

September 2022

Black hole X-ray binaries (BHXBs) are stellar systems composed of an accreting black hole and a dono...

Evolution of the accretion disk in black hole X-ray transients

Meyer-Hofmeister, E.
Meyer, F.
Max-Planck-Institut fuer Astrophysik, Garching (Germany)

January 2000

Several black hole X-ray transients have a very long recurrence time, decades of years. We study the...

Revealing the gamma-ray jet in a black hole binary

Martin J. Hardcastle

October 2016

Novel techniques in gamma-ray polarimetry allow gamma-ray emission from a black-hole binary in the M...

Why Do Black-Hole X-ray Binaries Tend to Be Transient?

Lasota, J P

November 1999

Black hole X-ray binaries are transient probably because their discs are subject to the same thermal...

The corona contracts in a black-hole transient

Kara, E.
Steiner, J. F.
Fabian, A. C.
Cackett, E. M.
Uttley, P.
Remillard, R. A.
Gendreau, K. C.
Arzoumanian, Z.
Altamirano, D.
Eikenberry, S.
Enoto, T.
Homan, J.
Neilsen, J.
Stevens, A. L.

January 2019

The geometry of the accretion flow around stellar-mass black holes can change on timescales of days ...

The formation of the black hole in the X-ray binary system V404 Cyg

Miller-Jones, J.C.A.
Jonker, P.G.
Nelemans, G.A.
Zwart, S. Portegies
Dhawan, V.
Brisken, W.
Gallo, E.
Rupen, M.P.

January 2008

Contains fulltext : 72479.pdf (author's version ) (Open Access)11 p

Tracking the evolution of the accretion flow in MAXI J1820+070 during its hard state with the JED-SAD model

Marino, A.
Barnier, S.
Petrucci, P.O.
del Santo, M.
Malzac, J.
Ferreira, J.
Marcel, G.
Segreto, A.
Motta, S.E.
d'Aì, A.
Di Salvo, T.
Guillot, S.
Russell, T.D.

January 2021

International audienceContext. X-ray binaries in outburst typically show two canonical X-ray spectra...

Black hole X-ray binaries: A new view on soft-hard spectral transitions

Meyer, F.
Meyer-Hofmeister, E. (Max-Planck-Institut fuer Astrophysik, Garching (Germany))
Academia Sinica, Kunming, YN (China). Yunnan Observatory)
Liu, B.F. (Max-Planck-Institut fuer Astrophysik, Garching (Germany)
Max-Planck-Institut fuer Astrophysik, Garching (Germany)

January 2000

SIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB...

Black hole soft X-ray transients: evolution of the cool disk and mass supply for the ADAF

Meyer-Hofmeister, E.
Meyer, F.
Max-Planck-Institut fuer Astrophysik, Garching (Germany)

January 1999

SIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB...

Analytical Model of Disk Evaporation and State Transitions in Accreting Black Holes

Cho, Hyerin
Narayan, Ramesh

June 2022

State transitions in black hole X-ray binaries are likely caused by gas evaporation from a thin accr...

The formation of black hole low-mass X-ray binaries: Through case B or case C mass transfer?

Nelemans, G.A.
Heuvel, E.P.J. van den

January 2001

Contains fulltext : 156202.pdf (preprint version ) (Open Access

Accretion disc coronae in black hole binaries.

Malzac, J.

December 2006

Most of the luminosity of accreting black hole is emitted in the X-ray band. This radiation is belie...

Black hole X-ray transients: mass accumulation in the disk - constraints for the viscosity

Meyer-Hofmeister, E.
Meyer, F.
Max-Planck-Institut fuer Astrophysik, Garching (Germany)

January 2000

The outburst cycles of black hole X-ray transients are now generally understood as caused by a therm...

Accretion disc coronae in black hole binaries

J Malzac

March 2020

Abstract. Most of the luminosity of accreting black hole is emitted in the X-ray band. This radiatio...

The Effect of Coronal Radiation on a Residual Inner Disk in the Low/Hard Spectral State of Black Hole X-ray Binary Systems

Liu, B.F.
Done, C.
Taam, R.E.

January 2011

Thermal conduction between a cool accretion disk and a hot inner corona can result in either evapora...

Wind-type outflows from black hole X-ray binary MAXI J1820+070: the near infrared view

Sánchez-Sierras, Javier
Muñoz-Darias, Teo

September 2022

Black hole X-ray binaries (BHXBs) are stellar systems composed of an accreting black hole and a dono...

Evolution of the accretion disk in black hole X-ray transients

Meyer-Hofmeister, E.
Meyer, F.
Max-Planck-Institut fuer Astrophysik, Garching (Germany)

January 2000

Several black hole X-ray transients have a very long recurrence time, decades of years. We study the...

Revealing the gamma-ray jet in a black hole binary

Martin J. Hardcastle

October 2016

Novel techniques in gamma-ray polarimetry allow gamma-ray emission from a black-hole binary in the M...

Why Do Black-Hole X-ray Binaries Tend to Be Transient?

Lasota, J P

November 1999

Black hole X-ray binaries are transient probably because their discs are subject to the same thermal...

The corona contracts in a black-hole transient

Kara, E.
Steiner, J. F.
Fabian, A. C.
Cackett, E. M.
Uttley, P.
Remillard, R. A.
Gendreau, K. C.
Arzoumanian, Z.
Altamirano, D.
Eikenberry, S.
Enoto, T.
Homan, J.
Neilsen, J.
Stevens, A. L.

January 2019

The geometry of the accretion flow around stellar-mass black holes can change on timescales of days ...

The formation of the black hole in the X-ray binary system V404 Cyg

Miller-Jones, J.C.A.
Jonker, P.G.
Nelemans, G.A.
Zwart, S. Portegies
Dhawan, V.
Brisken, W.
Gallo, E.
Rupen, M.P.

January 2008

Contains fulltext : 72479.pdf (author's version ) (Open Access)11 p

Tracking the evolution of the accretion flow in MAXI J1820+070 during its hard state with the JED-SAD model

Marino, A.
Barnier, S.
Petrucci, P.O.
del Santo, M.
Malzac, J.
Ferreira, J.
Marcel, G.
Segreto, A.
Motta, S.E.
d'Aì, A.
Di Salvo, T.
Guillot, S.
Russell, T.D.

January 2021

International audienceContext. X-ray binaries in outburst typically show two canonical X-ray spectra...

Black hole X-ray binaries: the transition from the cool thin disk to the coronal flow

Abstract

Extracted data

Black hole X-ray binaries: the transition from the cool thin disk to the coronal flow

Abstract

Extracted data

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