Publications by Katherine Blundell


Concepts in thermal physics

Oxford University Press, USA, 2006

S Blundell, KM Blundell

This modern introduction to thermal physics contains a step-by-step presentation of the key concepts. The text is copiously illustrated and each chapter contains several worked examples.


Extended inverse Compton enussion from distant powerful radio galaxies

ESA SP PUBL 604 (2006) 611-612

MC Erlund, AC Fabian, KM Blundell, A Celotti, C Crawford

Chandra observations of 3C432, 3C191 and B2 0902+34 are presented as part of an ongoing search for inverse-Compton scattering of the cosmic microwave background (CMB) from high redshift radio sources (Schwartz, 2000). The energy density of the CMB increases with redshift, z, as (1 + Z)(4), so the relatively high redshift of these powerful radio galaxies makes them good candidates for detecting extended inverse-Compton scattering along the radio jet axis: we do indeed detect radio-aligned X-ray emission.


Extended inverse compton emission from distant powerful radio galaxies

European Space Agency, (Special Publication) ESA SP 2 (2006) 611-612

MC Erlund, AC Fabian, KM Blundell, A Celotti, C Crawford

Chandra observations of 3C432, 3C 191 and B2 0902+34 are presented as part of an ongoing search for inverse-Compton scattering of the cosmic microwave background (CMB) from high redshift radio sources (Schwartz, 2000). The energy density of the CMB increases with redshift, z, as (1 + z)4, so the relatively high redshift of these powerful radio galaxies makes them good candidates for detecting extended inverse-Compton scattering along the radio jet axis: we do indeed detect radio-aligned X-ray emission.


Exploring the nature of weak Chandra sources near the Galactic Centre

AIP CONF PROC 797 (2005) 410-415

RM Bandyopadhyay, JCA Miller-Jones, KM Blundell, FE Bauer, P Podsiadlowski, QD Wang, S Rappaport, E Pfahl

We present results from the first near-IR imaging of the weak X-ray sources discovered in the Chandra/ACIS-I survey (Wang et al. 2002) towards the. Galactic Centre (GC). These 800 discrete sources, which contribute significantly to the GC X-ray emission, represent an important and previously unknown population within the Galaxy. From our VLT observations we will identify likely IR counterparts to a sample of the hardest sources, which am most likely X-ray binaries, With these data we can place constraints on the nature of the discrete weak X-ray source population of the GC.


A refined method for measuring jet speeds

Interacting Binaries: Accretion, Evolution, and Outcomes 797 (2005) 585-588

J Miller-Jones, K Blundell, P Duffy


Jet Velocity in SS 433: Its Anticorrelation with Precession-Cone Angle and Dependence on Orbital Phase

Astrophysical Journal Letters 622 (2005) L129-L132

KM Blundell, Michael G. Bowler


The distribution of radio plasma in time and space.

Philos Trans A Math Phys Eng Sci 363 (2005) 645-654

KM Blundell

The influence of jet-ejected plasma has been an important theme of this meeting; I draw attention to the prevalence of jet-ejected plasma, in particular that which has not been properly accounted for in the past. There are three strands to this paper: important emission which is prominent only at the lowest radio frequencies; relic radio plasma which must exist if even the most basic aspects of radio source evolutionary models are correct; and evidence that some 'radio-quiet' quasars could be FR-I radio sources.


The post-outburst radio evolution of Cygnus X-3

ASTR SOC P 340 (2005) 312-314

AJ Mioduszewski, MP Rupen, JCA Miller-Jones, KM Blundell

Cygnus X-3 is one of the most famous Galactic relativistic jet sources, often undergoing flares to 1 Jy or more. Here we present VLBA imaging at 15 and 22 GHz after the September 2001 outburst and contrast the one-sided nature of the VLBI jets with the two-sided jet seen in VLA images of this source.


The impact of active galaxies on the Universe at large - Preface

PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES 363 (2005) 611-612

J Binney, KM Blundell, JP Ostriker, SDM White


Cosmic ray transport and acceleration

PLASMA PHYS CONTR F 47 (2005) B667-B678

P Duffy, KM Blundell

We review the theory of cosmic ray transport and acceleration with an emphasis on the underlying plasma physics and examine how that theory can be applied to sources such as supernova remnants and giant radio galaxies. Starting with Fermi's original model for scattering off moving magnetized clouds, we discuss quasilinear transport theory and its application to the acceleration of particles at shock fronts. We discuss problems of injection and the excitation of MHD turbulence by the accelerated particles. In the diffusive limit and at strong shocks this mechanism produces a differential energy spectrum of N(E) (proportional to E-2. Recent observations of supernova remnants suggest that their spectra may be steeper than this value. We discuss the transport and acceleration of energetic particles in highly correlated magnetic field structures. In this case particles have an enhanced probability of escape from the shock as they are trapped on field lines and the resulting spectrum is steepened up to a value of 2.5. Fast particle transport also seems to be required by observations of the structures of giant radio galaxy lobes as a function of frequency.


Jets and outflows in microquasars

ASTR SOC P 330 (2005) 91-102

KM Blundell

I discuss the importance of studies of jets and outflows in the Galaxy from binary star systems, popularly known as microquasars. Because of the rapid timescales on which they evolve, pertinent observations of microquasar jets can help tighten up the theoretical framework in which jet properties of quasars can be interpreted. I draw attention to a new method for constraining jet speed which renders original approaches, which do not incorporate jet evolution, obsolete. I describe new results on two particular microquasars, SS 433 and Cygnus X-3. I compare and contrast the jet characteristics of these two microquasars, noting the persistent jet activity of SS 433 with the intermittent jet activity of Cygnus X-3.


Symmetry in the Changing Jets of SS 433 and Its True Distance from Us

Astrophysical Journal Letters 616 (2004) L159-L162

KM Blundell, Michael G. Bowler


Exploring the nature of weak Chandra sources near the galactic centre

Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias 20 (2004) 261-262

RM Bandyopadhyay, KM Blundell, P Podsiadlowski, JCA Miller-Jones, QD Wang, WN Brandt, S Rappaport, E Pfahl

We present early results from the first near-IR imaging of the weak X-ray sources discovered in the recent Chandra/ACIS-I survey towards the Galactic Centre (GC) (Wang et al. 2002). These ̃800 discrete sources, which contribute significantly to the GC X-ray emission, represent an important and previously unknown population within the Galaxy. From our VLT observations we will identify likely IR counterparts to a sample of the hardest sources, which are most likely X-ray binaries. With these data we can place constraints on the nature of the discrete weak X-ray source population of the GC. Once the data analysis is complete we will discuss our results in the context of binary population synthesis models. © Copyright 2004: IA, UNAM.


The 6C** sample and the highest redshift radio galaxies

(2004) 141-142

MJ Cruz, MJ Jarvis, KM Blundell, S Rawlings

We present a new radio sample, 6C** designed to find radio galaxies at z > 4 and discuss some of its near-infrared imaging follow-up results.


Near-infrared imaging and the K-z relation for radio galaxies in the 7C Redshift Survey 

Monthly Notices of the Royal Astronomical Society 339 (2003) 173-188

SG Rawlings, Blundell, K, Jarvis, M, Willott, C


A Relativistic Jet in the Radio-quiet Quasar PG 1407+263

Astrophysical Journal Letters 591 (2003) L103-L106

KM Blundell, Anthony J. Beasley, Geoffrey V. Bicknell


The mass of radio galaxies from low to high redshift

ESO ASTROPHY SYMP (2003) 148-153

MJ Jarvis, S Rawlings, S Eales, KM Blundell, CJ Willott

Using a new radio sample, 6C* designed to find radio galaxies at z > 4 along with the complete 3CRR and 6CE sample we extend the radio galaxy K - z relation to z similar to 4.5. The 6C* K - z data significantly improve delineation of the K - z relation for radio galaxies at high redshift (z > 2). In a spatially flat universe with a cosmological constant (Omega(M) = 0.3 and Omega(A) = 0.7), the most luminous radio sources appear to be associated with galaxies with a luminosity distribution with a high mean (approximate to 5L*), and a low dispersion (sigma similar to 0.5 mag) which formed their stars at epochs corresponding to z greater than or similar to 2.5).


The ruff of equatorial emission around the SS433 jets: its spectral index and origin

Proceedings of the 4th Microquasar Workshop (2003)

KM Blundell, MP Rupen, AJ Mioduszewski, TWB Muxlow, P Podsiadlowski

We present unique radio observations of SS433, using MERLIN, the VLBA, and the VLA, which allow us to, for the first time, properly image and derive a meaningful spectral index for the `ruff' of equatorial emission which surrounds SS433's jet. We interpret this smooth ruff as a wind-like outflow from the binary.


Lowering inferred cluster magnetic field strengths: The radio galaxy contributions

Astrophysical Journal 588 (2003) 143-154

L Rudnick, KM Blundell

We present a detailed examination of the relationship between the magnetic field structures and the variations in Faraday rotation across PK.S 1246-410, a radio source in the Centaurus cluster of galaxies, using data from Taylor, Fabian, & Alien. We find a significant relationship between the intrinsic position angle of the polarization and the local amount of Faraday rotation. The most plausible explanation is that most or all of the rotation is local to the source. We suggest that the rotations local to cluster radio galaxies may result either from thermal material mixed with the radio plasma, or from thin skins of warm, ionized gas in pressure balance with the observed galaxy or hot cluster atmospheres. We find that the contribution of any unrelated cluster rotation measure (RM) variations on scales of 2″-10″ are less than 25 rad m-2 the standard, although model-dependent, derivation of cluster fields would then lead to an upper limit of ≈0.4μG on these scales. Inspection of the distributions of rotation measure, polarization angle, and total intensity in 3C 75, 3C 465, and Cygnus A also shows source-related Faraday effects in some locations. Many effects can mask the signatures of locally dominated RMs, so the detection of even isolated correlations can be important, although difficult to quantify statistically. In order to use radio sources such as those shown here to derive cluster-wide magnetic fields, as is commonly done, one must first remove the local contributions. This is not possible at present.


Radio galaxy evolution: what you can learn from a brief encounter

NEW ASTRON REV 46 (2002) 75-87

KM Blundell, S Rawlings, CJ Willott, NE Kassim, R Perley

We describe the pitfalls encountered in deducing from classical double radio source observables (luminosity, spectral index, redshift and linear size) the essential nature of how these objects evolve. We discuss the key role played by hotspots in governing the energy distribution of the lobes they feed, and subsequent spectral evolution. We present images obtained using the new 74 MHz receivers on the VLA and discuss constraints which these enforce on models of the backflow and ages in classical doubles. (C) 2002 Elsevier Science B.V. All rights reserved.

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