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Rosse Telescope

Garret Cotter

Professor of Physics

Research theme

  • Astronomy and astrophysics
  • Particle astrophysics & cosmology

Sub department

  • Astrophysics

Research groups

  • Pulsars, transients and relativistic astrophysics
  • The Square Kilometre Array (SKA)
  • Gamma-ray astronomy
Garret.Cotter@physics.ox.ac.uk
Telephone: 01865 (2)73604
Denys Wilkinson Building, room Dalitz 4
  • About
  • Publications

Blazars in the Fermi Era: The OVRO 40-m Telescope Monitoring Program

(2010)

Authors:

Joseph L Richards, Walter Max-Moerbeck, Vasiliki Pavlidou, Oliver G King, Timothy J Pearson, Anthony CS Readhead, Rodrigo Reeves, Martin C Shepherd, Matthew A Stevenson, Lawrence C Weintraub, Lars Fuhrmann, Emmanouil Angelakis, J Anton Zensus, Stephen E Healey, Roger W Romani, Michael S Shaw, Keith Grainge, Mark Birkinshaw, Katy Lancaster, Diana M Worrall, Gregory B Taylor, Garret Cotter, Ricardo Bustos
More details from the publisher

Characteristics of Gamma-Ray Loud Blazars in the VLBA Imaging and Polarimetry Survey

(2010)

Authors:

JD Linford, GB Taylor, R Romani, SE Healey, JF Helmboldt, ACS Readhead, R Reeves, J Richards, G Cotter
More details from the publisher

The Balmer-dominated Bow Shock and Wind Nebula Structure of Gamma-ray Pulsar PSR J1741-2054

(2010)

Authors:

Roger W Romani, Michael S Shaw, Fernando Camilo, Garret Cotter, Gregory R Sivakoff
More details from the publisher

The extraordinary radio galaxy MRC B1221-423: probing deeper at radio and optical wavelengths

(2010)

Authors:

Helen M Johnston, Jess W Broderick, Garret Cotter, Raffaella Morganti, Richard W Hunstead
More details from the publisher

The extraordinary radio galaxy MRC B1221-423: Probing deeper at radio and optical wavelengths

Monthly Notices of the Royal Astronomical Society 407:2 (2010) 721-733

Authors:

HM Johnston, JW Broderick, G Cotter, R Morganti, RW Hunstead

Abstract:

We present optical spectra and high-resolution multiwavelength radio observations of the compact steep-spectrum radio source MRC B1221-423 (z = 0.1706). MRC B1221-423 is a very young (∼105 yr), powerful radio source which is undergoing a tidal interaction with a companion galaxy. We find strong evidence of interaction between the active galactic nucleus (AGN) and its environment. The radio morphology is highly distorted, showing a dramatic interaction between the radio jet and the host galaxy, with the jet being turned almost back on itself. H i observations show strong absorption against the nucleus at an infall velocity of ∼250 km s-1 compared to the stellar velocity, as well as a second, broader component which may represent gas falling into the nucleus. Optical spectra show that star formation is taking place across the whole system. Broad optical emission lines in the nucleus show evidence of outflow. Our observations confirm that MRC B1221-423 is a young radio source in a gas-rich nuclear environment, and that there was a time delay of a few times 100 Myr between the onset of star formation and the triggering of the AGN. © 2010 The Authors. Journal compilation © 2010 RAS.
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