Lunch (TTSO6)
Session details: Monday, 2012-04-09 02:25:00
Session details: Monday, 2012-04-09 02:25:00
Session details: Sunday, 2024-03-31 08:30:00, DISH2| Abstract The NACAA Farewell BBQ, being held at the famous “DISH”, is a chance to wind down at the end of a busy and exciting weekend. During the event, the Astral Award for best presenter will be announced and the handover will occur to the new Local Organising Committee…
Sat 11:00-12:30 Room: T1 11:00 Sarah Sweet – Star-forming dwarf galaxies in groups 11:30 Graeme Jenkinson – Double Stars; Real Science on a Budget 12:00 Tim Napier-Munn – Measuring Double Stars
Presenter(s): Mr Stephen Russell Session details: Saturday, 2010-04-03 05:30:00 Abstract The purpose of the NACAA Inc AGM is to elect five officers to serve on the national committee for the next two years. As well, the General Secretary and Treasurer will present short reports, and any other necessary business will be conducted, prior to the…
Presenter(s): Marnie Ogg Session details: Saturday, 2026-04-03 22:30:00 Abstract Around the world, artificial light at night is being redefined. No longer seen as harmless progress, it is now recognised as an environmental pressure, a scientific threat, and a public health concern. Governments are adopting light pollution guidelines, observatories are strengthening protection measures, and research continues…
Presenter(s): Mr Anthony Wesley Affiliation(s): Canberra Astronomical Society Session details: Friday, 2010-04-02 02:30:00 Abstract High resolution planetary imaging involves capturing a large amount of raw video data and then reducing this via several software techniques and applications to a finished colour image. This workshop will walk through these software packages and demonstrate various techniques relevant…
Affiliation(s): UQ Session details: Saturday, 2012-04-07 01:00:00, TBA Abstract We have discovered a new type of galaxy group with very active star formation. Usually, groups of galaxies have low star formation rates because there is not much fuel available to form stars. The observed high rates of star formation in our groups could be explained…