activity
19982006
most citedThe radio luminosity of persistent X-ray binaries

146 citations · 238 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph2006★ 85 cited

SN 2004A: Another Type II-P Supernova with a Red Supergiant Progenitor

M. A. Hendry, S. J. Smartt, R. M. Crockett +8

We present a monitoring study of SN 2004A and probable discovery of a progenitor star in pre-explosion HST images. The photometric and spectroscopic monitoring of SN 2004A show tha…

astro-ph2005

Microlensing of Circumstellar Envelopes. III. Line profiles from stellar winds in homologous expansion

M. A. Hendry, R. Ignace, H. M. Bryce

This paper examines line profile evolution due to the linear expansion of circumstellar material obsverved during a microlensing event. This work extends our previous papers on emi…

astro-ph2000★ 4 cited

Analytic Inversion of Emission Lines of Arbitrary Optical Depth for the Structure of Supernova Ejecta

R. Ignace, M. A. Hendry

We derive a method for inverting emission line profiles formed in supernova ejecta. The derivation assumes spherical symmetry and homologous expansion (i.e., ), is…

astro-ph2000★ 146 cited

The radio luminosity of persistent X-ray binaries

R. P. Fender, M. A. Hendry

We summarise all the reported detections of, and upper limits to, the radio emission from persistent (i.e. non-transient) X-ray binaries. A striking result is a common mean observe…

astro-ph1999★ 3 cited

A robust method for measuring the Hubble parameter

M. A. Hendry, S. Rauzy

We obtain a robust, non-parametric, estimate of the Hubble constant from galaxy linear diameters calibrated using HST Cepheid distances. Our method is independent of the parametric…

astro-ph1998

The Polarisation Signatures of Microlensing

A. M. Newsam, J. F. L. Simmons, M. A. Hendry +1

It has already been shown that microlensing can give rise to a non-zero variable polarisation signal. Here we use realistic simulations to demonstrate the additional information th…