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NOVAE SEARCH GROUP. Team leaders: Sara Garzia Giovanni Sostero Group members: Maja Hren Ana Bonaca Natko Bajić. Aim of the group: Learn how to prepare a search program Optimize the method with the available instrumentation Refine the method while operating
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NOVAE SEARCH GROUP Team leaders: Sara Garzia Giovanni Sostero Group members: Maja Hren Ana Bonaca Natko Bajić VSA Novae group
Aim of the group: • Learn how to prepare a search program • Optimize the method with the available instrumentation • Refine the method while operating • Enjoy the VSA School VSA Novae group
TOPICS SUMMARY • An introduction to nova phenomenon • Classical novae search program at the 2002 VSA • Recurrent novae monitoring programat the 2002 VSA VSA Novae group
Field of Nova Aquilae 1999 before explosion VSA Novae group
KA-BOOM!!!!!!!!!! VSA Novae group
The expanding shell of material after a nova outburst Accretion hydrogen disc around white dwarf VSA Novae group
DISTRIBUTION OF NOVAE VSA Novae group
THE FREQUENCY VSA Novae group
LIGHT CURVE VSA Novae group
FIELDS OF VSA Novae group
ACQUISITION EQUIPMENT • TELEOBJECTIVES • 80mm-field of view 43°x43° limiting magnitude 12 at best • 180mm- field of view 20°x20° limiting magnitude 13.5 at best • OUR OBSERVATIONS • (180mm f/2.8) VSA Novae group
NEGATIVES PRODUCTION • developing TMAX 400 film • after film was dry, we cut each negative • we put them into bags we made (archive) • inspecting them VSA Novae group
BLINKING VSA Novae group
ACTUAL BLINKING VSA Novae group
RESULTS • 5 nights of work, an average of 6 fields each night • Some 10 variable stars identified, a couple of them seems to be new • Hundredes of dustgrains discovered • The search has proved to be potentially effective • We need just more time to search… VSA Novae group
RECURRENT NOVAE PROGRAM VSA Novae group
HOW TO RECOGNIZE A RECURRENT NOVA? VSA Novae group
OUR PROGRAM VSA Novae group
DISTRIBUTION VSA Novae group
EQUIPMENT VSA Novae group
BC Cassiopeae VSA Novae group
LS Andromedae VSA Novae group
We simply haven’t enough time to draw any conslusion More telescope time is needed… VSA Novae group
REFERENCES: Classical Novae, M.F. Bode and A. Evans editors, J. Wiley & Sons, 1989 www.aavso.org vsnet.kusastro.kyoto-u.ac.jp www.arksky.org/SuperNovae.htm ACKOWLEDGMENTS Višnjan Observatory staff Korado, Ivan and Luca VSA Novae group