Dmitry Monin

HD 35502: a hierarchical triple system with a magnetic B5IVpe primary

We present our analysis of HD~35502 based on high- and medium-resolution spectropolarimetric observations. Our results indicate that the magnetic B5IVsnp star is the primary component of a spectroscopic triple system and that it has an effective temperature of

Gemini high-resolution optical spectrograph conceptual design

18.4\pm0.6\,{\rm kK}

The Magnetic Early B-type Stars I: Magnetometry and Rotation

, a mass of

First science results with a new, inexpensive liquid crystal polarimeter module for the DAO 1.8m telescope

5.7\pm0.6\,M_\odot

Confirming HD 23478 As A New Magnetic B Star Hosting An Hα-Bright Centrifugal Magnetosphere

, and a polar radius of

The DAO Liquid Crystal Spectropolarimeter dimaPol

3.0^{+1.1}_{-0.5}\,R_\odot

The Dominion Astrophysical Observatory Magnetic Field Survey (DMFS)

. The two secondary components are found to be essentially identical A-type stars for which we derive effective temperatures (

Spectropolarimetry with the DAO 1.8-m telescope

8.9\pm0.3\,{\rm kK}

Possible Detection of Weak Magnetic Fields in Two White Dwarfs, Including the Pulsating WD 1647+591

), masses (

Magnetism of White Dwarfs (intermediate results of a survey for kilogauss magnetic fields in white dwarfs)

2.1\pm0.2\,M_\odot