Pulsars, transients and relativistic astrophysics

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The progenitor mass of the Type IIP supernova SN 2004et from late-time spectral modeling

(2012)

Authors:

Anders Jerkstrand, Claes Fransson, Kate Maguire, Stephen Smartt, Mattias Ergon, Jason Spyromilio
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Future Science Prospects for AMI

(2012)

Authors:

Keith Grainge, Paul Alexander, Richard Battye, Mark Birkinshaw, Andrew Blain, Malcolm Bremer, Sarah Bridle, Michael Brown, Richard Davis, Clive Dickinson, Alastair Edge, George Efstathiou, Robert Fender, Martin Hardcastle, Jennifer Hatchell, Michael Hobson, Matthew Jarvis, Benjamin Maughan, Ian McHardy, Matthew Middleton, Anthony Lasenby, Richard Saunders, Giorgio Savini, Anna Scaife, Graham Smith, Mark Thompson, Glenn White, Kris Zarb-Adami, James Allison, Jane Buckle, Alberto Castro-Tirado, Maria Chernyakova, Roger Deane, Farhan Feroz, Ricardo Genova Santos, David Green, Diana Hannikainen, Ian Heywood, Natasha Hurley-Walker, Ruediger Kneissl, Karri Koljonen, Shrinivas Kulkarni, Sera Markoff, Carrie MacTavish, Michael McCollough, Simone Migliari, Jon M Miller, James Miller-Jones, Malak Olamaie, Zsolt Paragi, Timothy Pearson, Guy Pooley, Katja Pottschmidt, Rafael Rebolo, John Richer, Julia Riley, Jerome Rodriguez, Carmen Rodriguez-Gonzalvez, Anthony Rushton, Petri Savolainen, Paul Scott, Timothy Shimwell, Marco Tavani, John Tomsick, Valeriu Tudose, Kurt van der Heyden, Alexander van der Horst, Angelo Varlotta, Elizabeth Waldram, Joern Wilms, Andrzej Zdziarski, Jonathan Zwart, Yvette Perrott, Clare Rumsey, Michel Schammel
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Stellar Mass Black Holes and Ultraluminous X-Ray Sources

(2012)

Authors:

Rob Fender, Tomaso Belloni
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Stellar-mass black holes and ultraluminous x-ray sources.

Science 337:6094 (2012) 540-544

Authors:

Rob Fender, Tomaso Belloni

Abstract:

We review the likely population, observational properties, and broad implications of stellar-mass black holes and ultraluminous x-ray sources. We focus on the clear empirical rules connecting accretion and outflow that have been established for stellar-mass black holes in binary systems in the past decade and a half. These patterns of behavior are probably the keys that will allow us to understand black hole feedback on the largest scales over cosmological time scales.
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Details from ArXiV

Future Science Prospects for AMI

ArXiv e-prints (2012)

Authors:

K Grainge, P Alexander, R Battye, M Birkinshaw, A Blain, M Bremer, S Bridle, M Brown, R Davis, C Dickinson, A Edge, G Efstathiou, R Fender, M Hardcastle, J Hatchell, M Hobson, M Jarvis, B Maughan, I McHardy, M Middleton, A Lasenby, R Saunders, G Savini, A Scaife, G Smith, M Thompson, G White, K Zarb-Adami, J Allison, J Buckle, A Castro-Tirado, M Chernyakova, R Deane, F Feroz, R Genova Santos, D Green, D Hannikainen, I Heywood, N Hurley-Walker, R Kneissl, K Koljonen, S Kulkarni, S Markoff, C MacTavish, M McCollough, S Migliari, JM Miller, J Miller-Jones, M Olamaie, Z Paragi, T Pearson, G Pooley, K Pottschmidt, R Rebolo, J Richer, J Riley, J Rodriguez, C Rodriguez-Gonzalvez, A Rushton, P Savolainen, P Scott, T Shimwell, M Tavani, J Tomsick, V Tudose, K van der Heyden, A van der Horst, A Varlotta, E Waldram, J Wilms, A Zdziarski, J Zwart, Y Perrott, C Rumsey, M Schammel
Details from ArXiV