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INTERVIEWS

Ronald Downes

Principle author of the Downes et al, Online Catalog and Atlas of Cataclysmic Variables, shines a light on the process for inclusion in the catalog for CVnet observers.

Boris Gaensicke

Dr. Boris Gaensicke, an assistant professor in the Department of Physics at the University of Warwick, England, discusses cataclysmic variables, observational population studies of CVs and magnetic CVs with Gary Poyner in this exclusive CVnet interview.

Arne Henden

The Director of the AAVSO talks with CVnet about the future of CV research, CCD and visual observations, observing campaigns and Pro-Am collaboration.

Steve Howell

Steve Howell, an astronomer at the WIYN Observatory located on Kitt Peak near Tucson, Arizona, discusses polars, magnetic fields and the nature of the secondary stars in these systems.

Guy Hurst

Guy Hurst, past President of the British Astronomical Association and Editor of "The Astronomer" magazine, discusses Pro-Am collaboration.

Koji Mukai

Koji Mukai, a Ph.D astronomer working for the NASA Goddard Space Flight Center, discusses intermediate polars, magnetic CVs that confound our attempts to understand them in many ways.

Joe Patterson

Joe Patterson, professor of astronomy at Columbia University, talks with CVnet about the Center for Backyard Astrophysics (CBA) and their CV activities.

Gary Poyner

Gary, an English amateur, talks about the Recurrent Objects Programme, a program to monitor for outbursts of poorly understood cataclysmic variables and other eruptive stars.

Paula Szkody

Paula, professor of astronomy at the University of Washington, talks about the CVs being discovered by the Sloan Digital Sky Survey.

ARTICLES

SDSS CVs for Amateur Telescopes and CCDs

Now that five papers on CVs in the Sloan Digital Sky Survey (SDSS) are publicly available, I thought it was time to evaluate these discoveries to search out the ones most likely to pay dividends for amateurs monitoring them with CCDs on .5m telescopes and smaller.

Small Scope Sampler

CVs suitable for observing with small telescopes!

Recurrent Novae

These cataclysmic variables grab our attention and spark our imaginations because of the incredible amplitude of their outbursts, typically 8-12 magnitudes, and the rarity of these spectacular events.

UGZ or not UGZ?

The old adage "you can’t believe everything you read" was never truer than for cataclysmic variables of the type UGZ.

From the CVnet 100 year birthday celebration of U Gem

J. R. Hind The Discoverer of U Geminorum

Historical observations of U Gem in the BAA VSS Database

U Gem and the AAVSO

Suspected Variables in the field of U Gem