activity
20002020
most citedE-BOSS: an Extensive stellar BOw Shock Survey. I: Methods and First Catalogue

110 citations · 414 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2020★ 2 cited

COBRaS: The e-MERLIN 21 cm Legacy survey of Cygnus OB2

J. C. Morford, D. M. Fenech, R. K. Prinja +12

The role of massive stars is central to an understanding of galactic ecology. It is important to establish the details of how massive stars provide radiative, chemical, and mechani…

astro-ph.SR2017★ 1 cited

Photometric Variability of the mCP Star CS Vir: Evolution of the Rotation Period

Dogus Ozuyar, H. Tugca Sener, Ian R. Stevens

The aim of this study is to accurately calculate the rotational period of CS\,Vir by using {\sl STEREO} observations and investigate a possible period variation of the star with th…

astro-ph.SR2014★ 15 cited

Amplitude variability in satellite photometry of the non-radially pulsating O9.5V star zeta Oph

Ian D. Howarth, K. J. F. Goss, I. R. Stevens +2

We report a time-series analysis of satellite photometry of the non-radially pulsating Oe star zeta Oph, principally using data from SMEI obtained 2003--2008, but augmented with MO…

astro-ph.SR2011★ 110 cited

E-BOSS: an Extensive stellar BOw Shock Survey. I: Methods and First Catalogue

C. S. Peri, P. Benaglia, D. P. Brookes +2

Context: Bow shocks are produced by many astrophysical objects where shock waves are present. Stellar bow shocks, generated by runaway stars, have been previously detected in small…

astro-ph.SR2011★ 12 cited

The nearby eclipsing stellar system delta Velorum. II. First reliable orbit for the eclipsing pair

T. Pribulla, A. Merand, P. Kervella +8

Context. The nearby multiple system delta Velorum contains a widely detached eclipsing binary and a third component. Aims. We take advantage of this system offering the opportunity…

astro-ph2008★ 9 cited

SMEI observations of previously unseen pulsation frequencies in gamma Doradus

N. J. Tarrant, W. J. Chaplin, Y. P. Elsworth +2

Aims: As g-mode pulsators, gamma-Doradus-class stars may naively be expected to show a large number of modes. Taking advantage of the long photometric time-series generated by the…