Truncated disc versus extremely broad iron line in XTE J1650-500

Done, C.; Gierliński, M.

doi:10.1111/j.1365-2966.2005.09968.x

A Deep 0.3-10 keV Spectrum of the H$_2$O Maser Galaxy IC 2560 (2008)
Journal Article
Tilak, A., Greenhill, L., Done, C., & Madejski, G. (2008). A Deep 0.3-10 keV Spectrum of the H$_2$O Maser Galaxy IC 2560. Astrophysical Journal, 678, 701-711. https://doi.org/10.1086/529537

Funnel wall jets and the nature of the soft X-ray excess (2008)
Journal Article
Schurch, N., & Done, C. (2008). Funnel wall jets and the nature of the soft X-ray excess. Monthly Notices of the Royal Astronomical Society: Letters, 386, L1-L4. https://doi.org/10.1111/j.1745-3933.2007.00395.x

On why the iron K-shell absorption in AGN is not a signature of the local warm/hot intergalactic medium (2008)
Journal Article
Reeves, J., Done, C., Pounds, K., Terashima, Y., Hayashida, K., Anabuki, N., …Turner, M. (2008). On why the iron K-shell absorption in AGN is not a signature of the local warm/hot intergalactic medium. Monthly Notices of the Royal Astronomical Society: Letters, 385, L108-L112. https://doi.org/10.1111/j.1745-3933.2008.00443.x

High-energy X-ray spectra of Seyferts and Unification schemes for active galactic nuclei (2008)
Journal Article
Middleton, M., Done, C., & Schurch, N. (2008). High-energy X-ray spectra of Seyferts and Unification schemes for active galactic nuclei. Monthly Notices of the Royal Astronomical Society, 383, 1501-1505. https://doi.org/10.1111/j.1365-2966.2007.12648.x

Suzaku Wide-Band X-Ray Spectroscopy of the Seyfert2 AGN in NGC 4945 (2008)
Journal Article
Itoh, T., Done, C., Makishima, K., Madejski, G., Awaki, H., Gandhi, P., …Yaqoob, T. (2008). Suzaku Wide-Band X-Ray Spectroscopy of the Seyfert2 AGN in NGC 4945

Modelling the behaviour of accretion flows in x-ray binaries (2007)
Journal Article
Done, C., Gierlinski, M., & Kubota, A. (2007). Modelling the behaviour of accretion flows in x-ray binaries. Astronomy and Astrophysics Review, 15(1), 1-66. https://doi.org/10.1007/s00159-007-0006-1

We review how the recent increase in X-ray and radio data from black hole and neutron star binaries can be merged together with theoretical advances to give a coherent picture of the physics of the accretion flow in strong gravity. Both long term X-r... Read More about Modelling the behaviour of accretion flows in x-ray binaries.

Analysing the atolls: X-ray spectral transitions of accreting neutron stars. (2007)
Journal Article
Gladstone, J., Done, C., & Gierlinski, M. (2007). Analysing the atolls: X-ray spectral transitions of accreting neutron stars. Monthly Notices of the Royal Astronomical Society, 378(1), 13-22. https://doi.org/10.1111/j.1365-2966.2007.11675.x

We systematically analyse all the available X-ray spectra of disc accreting neutron stars (atolls and millisecond pulsars) from the RXTE data base. We show that while all these have similar spectral evolution as a function of mass accretion rate, the... Read More about Analysing the atolls: X-ray spectral transitions of accreting neutron stars..

Can the soft excess in AGN originate from disc reflection? (2007)
Journal Article
Done, C., & Nayakshin, S. (2007). Can the soft excess in AGN originate from disc reflection?. Monthly Notices of the Royal Astronomical Society: Letters, 377(1), L59-L63

Suzaku Observation of Two Ultraluminous X-Ray Sources in NGC 1313 (2007)
Journal Article
Mizuno, T., Miyawaki, R., Ebisawa, K., Kubota, A., Miyamoto, M., Winter, L. M., …Terashima, Y. (2007). Suzaku Observation of Two Ultraluminous X-Ray Sources in NGC 1313. Publications of Astronomical Society of Japan, 59, 257-267

What is the origin of the soft excess in active galactic nuclei? (2007)
Journal Article
Sobolewska, M., & Done, C. (2007). What is the origin of the soft excess in active galactic nuclei?. Monthly Notices of the Royal Astronomical Society, 374(1), 150-158. https://doi.org/10.1111/j.1365-2966.2006.11117.x

We investigate the nature of the soft excess below 1 keV observed in active galactic nuclei. We use the XMM–Newton data of the low-redshift, optically bright quasar, PG 1211+143, and we compare it with the narrow-line Seyfert 1 galaxy, 1H 0707−495, w... Read More about What is the origin of the soft excess in active galactic nuclei?.

Suzaku Discovery of Iron Absorption Lines in Outburst Spectra of the X-Ray Transient 4U 1630-472 (2007)
Journal Article
Kubota, A., Dotani, T., Cottam, J., Kotani, T., Done, C., Ueda, Y., …Angelini, L. (2007). Suzaku Discovery of Iron Absorption Lines in Outburst Spectra of the X-Ray Transient 4U 1630-472. Publications of Astronomical Society of Japan, 59, 185-198

The iron K feature in narrow line Seyfert 1 galaxies: evidence for a P Cygni profile? (2007)
Journal Article
Done, C., Sobolewska, M., Gierlinski, M., & Schurch, N. (2007). The iron K feature in narrow line Seyfert 1 galaxies: evidence for a P Cygni profile?. Monthly Notices of the Royal Astronomical Society: Letters, 374(1), L15-L19

Black hole spin in GRS 1915+105. (2006)
Journal Article
Middleton, M., Done, C., Gierliński, M., & Davis, S. (2006). Black hole spin in GRS 1915+105. Monthly Notices of the Royal Astronomical Society, 373(1), 1004-1012. https://doi.org/10.1111/j.1365-2966.2006.11077.x

Microquasars are galactic black hole binary systems with radio jets which can sometimes be spatially resolved to show superluminal motion. The first and best known of this class of objects is GRS 1915+105, the brightest accreting source in our Galaxy... Read More about Black hole spin in GRS 1915+105..

X-Ray Emission from Megamaser Galaxy IC 2560 (2006)
Presentation / Conference Contribution
Madejski, G., Done, C., Zycki, P., & Greenhill, L. (2006, December). X-Ray Emission from Megamaser Galaxy IC 2560

The decline and fall of GRS 1915+105: the end is nigh? (2006)
Presentation / Conference Contribution
Truss, M., & Done, C. (2006, December). The decline and fall of GRS 1915+105: the end is nigh?

Disc-corona energetics in the very high state of Galactic black holes (2006)
Journal Article
Done, C., & Kubota, A. (2006). Disc-corona energetics in the very high state of Galactic black holes. Monthly Notices of the Royal Astronomical Society, 371(1), 1216-1230

Failed disc winds: a physical origin for the soft X-ray excess? (2006)
Journal Article
Schurch, N., & Done, C. (2006). Failed disc winds: a physical origin for the soft X-ray excess?. Monthly Notices of the Royal Astronomical Society, 371(1), 81-92. https://doi.org/10.1111/j.1365-2966.2006.10645.x

Energy-dependent variability and the origin of the soft X-ray excess in active galactic nuclei (2006)
Journal Article
Gierliński, M., & Done, C. (2006). Energy-dependent variability and the origin of the soft X-ray excess in active galactic nuclei. Monthly Notices of the Royal Astronomical Society: Letters, 371(1), L16-L20

Testing Accretion Disk Theory in Black Hole X-Ray Binaries (2006)
Journal Article
Davis, S. W., Done, C., & Blaes, O. M. (2006). Testing Accretion Disk Theory in Black Hole X-Ray Binaries. Astrophysical Journal, 647(1), 525-538. https://doi.org/10.1086/505386

Truncated disc versus extremely broad iron line in XTE J1650-500 (2006)
Journal Article
Done, C., & Gierliński, M. (2006). Truncated disc versus extremely broad iron line in XTE J1650-500. Monthly Notices of the Royal Astronomical Society, 367(2), 659-668. https://doi.org/10.1111/j.1365-2966.2005.09968.x

There is growing evidence from both spectral and timing properties that there is a truncated inner accretion disc in low mass accretion rate Galactic black hole systems. The detection of extremely smeared relativistic iron lines in some of these syst... Read More about Truncated disc versus extremely broad iron line in XTE J1650-500.

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