The evolving polarized jet of black hole candidate swift J1745-26
Monthly Notices of the Royal Astronomical Society 437:4 (2014) 3265-3273
Abstract:
Swift J1745-26 is an X-ray binary towards the Galactic Centre that was detected when it went into outburst in 2012 September. This source is thought to be one of a growing number of sources that display 'failed outbursts', in which the self-absorbed radio jets of the transient source are never fully quenched and the thermal emission from the geometrically thin inner accretion disc never fully dominates the X-ray flux. We present multifrequency data from the Very Large Array, Australia Telescope Compact Array and Karoo Array Telescope (KAT- 7) radio arrays, spanning the entire period of the outburst. Our rich data set exposes radio emission that displays a high level of large-scale variability compared to the X-ray emission and deviations from the standard radio-X-ray correlation that are indicative of an unstable jet and confirm the outburst's transition from the canonical hard state to an intermediate state. We also observe steepening of the spectral index and an increase of the linear polarization to a large fraction (50 per cent) of the total flux, as well as a rotation of the electric vector position angle. These are consistent with a transformation from a self-absorbed compact jet to optically thin ejecta - the first time such a discrete ejection has been observed in a failed outburst - and may imply a complex magnetic field geometry. © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.The superluminous supernova PS1-11ap: bridging the gap between low and high redshift
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 437:1 (2014) 656-674
Transient astrophysics with the square kilometre array
Proceedings of Science 9-13-June-2014 (2014)
Abstract:
This chapter provides an overview of the possibilities for transient and variable-source astrophysics with the Square Kilometre Array. While subsequent chapters focus on the astrophysics of individual events, we focus on the broader picture, and how to maximise the science coming from the telescope. The SKA as currently designed will be a fantastic and ground-breaking facility for radio transient studies, but the scientifc yield will be dramatically increased by the addition of (i) near-real-time commensal searches of data streams for events, and (ii) on occasion, rapid robotic response to Target-of-Opprtunity style triggers.An Overview of Jets and Outflows in Stellar Mass Black Holes
Chapter in The Physics of Accretion onto Black Holes, Springer Nature 49 (2014) 323-337
On the origin of cyclotron lines in the spectra of X-ray pulsars
EPJ Web of Conferences EDP Sciences 64 (2014) 02005