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astro-ph2000

Microlensing extended stellar sources

H M Bryce, M A Hendry

We have developed a code to compute multi-colour microlensing lightcurves for extended sources, including the effects of limb darkening and photospheric star spots as a function of…

astro-ph1999

What can we learn from the fluxes of 1.2 Jy IRAS sample?

Stephane Rauzy, Martin Hendry

We present a new method for fitting peculiar velocity models to complete flux limited magnitude-redshifts catalogues, using the luminosity function of the sources as a distance ind…

astro-ph1998

Microlensing of Circumstellar Envelopes I. Simplified considerations for diagnosing radial and azimuthal flow

R. Ignace, M. A. Hendry

This paper presents first results on the line profile shapes from a circumstellar envelope in bulk motion as modified by a microlensing event. Only geometrically and optically thin…

astro-ph1997

One Arc Degree Core Substructure of the Virgo Cluster

A. R. Petrosian, V. G. Gurzadyan, M. A. Hendry +1

The results of an analysis of the substructure of 1 degree field galaxies of the Virgo cluster by means of the S-tree technique developed by Gurzadyan et al, are represented. The e…

astro-ph1996

Cepheids, supernovae and the value of

M. A. Hendry, S. M. Kanbur

The calibration of the Type Ia supernova distances using HST observations of Cepheid variables is discussed. A new maximum likelihood method of calibration is applied to derive the…

astro-ph1995

On improved Cepheid distance estimators

Shashi M. Kanbur, Martin A. Hendry

In this paper, we derive a physical argument for the existence of Period-luminosity and period-luminosity-colour relations at maximum light. We examine in detail a sample of Cephei…