Pulsars, transients and relativistic astrophysics

Research group

Research theme

Sub department

About

Population synthesis studies of isolated neutron stars with magnetic field decay

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 401:4 (2010) 2675-2686

Authors:

SB Popov, JA Pons, JA Miralles, PA Boldin, B Posselt
More details from the publisher

The Commensal Real-time ASKAP Fast Transients (CRAFT) survey

(2010)

Authors:

Jean-Pierre Macquart, the CRAFT collaboration, :, M Bailes, NDR Bhat, GC Bower, JD Bunton, S Chatterjee, T Colegate, JM Cordes, L D'Addario, A Deller, R Dodson, R Fender, K Haines, P Hall, C Harris, A Hotan, S Johnston, DL Jones, M Keith, JY Koay, TJW Lazio, W Majid, T Murphy, R Navarro, C Phillips, P Quinn, RA Preston, B Stansby, I Stairs, B Stappers, L Staveley-Smith, S Tingay, D Thompson, W van Straten, K Wagstaff, M Warren, R Wayth, L Wen
More details from the publisher

Powerful jets from accreting black holes: evidence from the optical and infrared

(2010)

Authors:

DM Russell, RP Fender
More details from the publisher

Two types of shock in the hotspot of the giant quasar 4C74.26: a high-resolution comparison from Chandra, Gemini & MERLIN

ArXiv 1001.1063 (2010)

Authors:

Mary Erlund, Andy Fabian, Katherine Blundell, Carolin Crawford, Paul Hirst

Abstract:

New Chandra observations have resolved the structure of the X-ray luminous southern hotspot in the giant radio quasar 4C74.26 into two distinct features. The nearer one to the nucleus is an extremely luminous peak, extended some 5 kpc perpendicular to the orientation of the jet; 19 kpc projected further away from the central nucleus than this is a fainter X-ray arc having similar symmetry. This arc is co-spatial with near-IR and optical emission imaged with Gemini, and radio emission imaged with MERLIN. The angular separation of the double shock structure (itself ~19 kpc or 10 arcsec in size) from the active nucleus which fuels them of ~550 kpc is a reminder of the challenge of connecting "unidentified" hard X-ray or Fermi sources with their origins.
Details from ArXiV
More details from the publisher

Two types of shock in the hotspot of the giant quasar 4C74.26: a high-resolution comparison from Chandra, Gemini & MERLIN

(2010)

Authors:

Mary Erlund, Andy Fabian, Katherine Blundell, Carolin Crawford, Paul Hirst
More details from the publisher