Dear all, I would like to forward the information on the IAU Colloquium 193, which is related to the variable stars. --- % Toshihito ISHIDA, Ph. D., Astrophysicist e-mail: ishida@nhao.go.jp % Nishi-Harima Astronomical Observatory, Sayo-cho, Hyogo 679-5313, JAPAN % Tel: +81-790-82-3886 ext. 142 Telefax: +81-790-82-3514 > ---------------------------------------------------------------------- > First Announcement > IAU Colloquium 193 > ---------------------------------------------------------------------- > Variable stars in the Local Group > > 6-11 July 2003, Christchurch, New Zealand > > Web page: http://www.vuw.ac.nz/scps/IAU193 > Conference e-mail: iau193@cont.canterbury.ac.nz > > *** If you would like to receive further information on this > conference, please indicate your interest by returning the > form at the end of this e-mail before 1 November 2002 *** > ---------------------------------------------------------------------- > > Dear Colleagues, > > We are very pleased to announce IAU Colloquium 193 "Variable stars in the > Local Group" to be held in Christchurch, New Zealand from 6-11 July 2003. > > This conference will immediately precede the IAU General Assembly to be > held nearby (3 hour flight) in Sydney, Australia (www.astronomy2003.com) > and will thus allow researchers to attend both meetings easily. > > The title and major theme of this meeting is stellar variability in the > Local Group and it follows by two years the highly successful Leuven > pulsation IAU colloquium. The theories of stellar structure and evolution > underpin all of stellar, galactic and extra-galactic astrophysics, so it > is appropriate that astronomers working in stellar pulsation meet > biennially to discuss advances in our field - from the structure of > crystallized white dwarf cores to the complex 3D interactions of AGB > stars with their envelopes in pre-planetary nebulae stages; from main > sequence p-mode and g-mode pulsators to exotic cases of tidally driven > variability; from the basic microscopic physics of astrophysical plasmas, > such as equations of state, opacities and radiative diffusion, to the > complex hydrodynamical phenomena of convection and circulation which > determine the chemical constitution of stars. > > The Local Group offers samples of all classes of variable stars, generally > with good information about distance and chemical composition from the > membership of the stars in various components of the Group. It provides > an environment in which we can study individual stars without the large > uncertainties in their distances that often plagues Galactic studies. > This is an essential stepping stone between the detailed understanding > of individual stars and the broader understanding of populations in > more distant galaxies. Eclipsing binary star distance determinations > in the Local Group will be contrasted with the results from the pulsating > star technique. > > With the recent dramatic advances in the observational material from the > new generation of large telescopes and the availability of large-scale > surveys, this provides an excellent opportunity for testing our > theoretical understanding of these stars and for generating discussion of > the implications and applications of stellar variability. The proposed > Colloquium is expected to yield substantial advances in these areas. > > The conference will cover the following major topics: > > - What variable stars tell us about the Local Group > - Variable stars as tracers of different stellar populations > (including galactic and globular clusters, LMC/SMC clusters and local > group galaxies) > - Early type stars: B, A and F pulsators > - Binary stars and pulsation > - Red Giants, Miras, post-AGB stars and proto-planetary nebulae > - Chemical composition of variable stars > - New theoretical developments in stellar pulsation/variability > - Evolutionary and pulsation properties of variable stars > - Our future in Space > > Presentations will include invited reviews, contributed talks and poster > papers. The second announcement and the call for scientific papers will be > sent out in December 2002. > > Invited speakers include: J. Christensen-Dalsgaard (Denmark), > A. Aparicio (Spain), K. Stanek (USA), A. Udalski (Poland), M. Catelan > (Chile), H. Habing (Netherlands), P. De Cat (Belgium), L. Bigot (France), > E. Guinan (USA), B. Willems (UK), T. Tanabe (Japan), M. Feast (S. Africa), > S. Vauclair (France), G. Fontaine (Canada), D. Dearborn (USA), > S. Cassisi (Italy), W. Lawson (Australia), J. Matthews (Canada), > C. Catala (France), S. Kawaler (USA). > > The conference will be held on the campus of the University of Canterbury, > in the city of Christchurch. Christchurch is the largest city in New > Zealand's South Island and offers many places of interest including museums, > an international Antarctic Centre, excellent botanical gardens and > numerous restaurants and cafes. Christchurch is ideally situated for > day-length activities including skiing, whale watching, bungy jumping, jet > boating and wine tours. The majestic Southern Alps are only a 1.5 hour > drive from Christchurch and offer some of the best ski-fields in New > Zealand. > > The Christchurch climate is temperate, with a mean temperature range for > July of 2 - 12 C -- the days are likely to be cool, clear and sunny, > although some rain is also probable at this time of year. (For further > information on Christchurch, see the following web page and related links: > http://www.conference.canterbury.ac.nz/chchinfo.htm) > > ------------------------------------------------------------------ > At this time you are invited to send expressions of interest using > the form at the end of this e-mail. Return to: > iau193@cont.canterbury.ac.nz by 1 November 2002 > ------------------------------------------------------------------ > > We also ask you to pass on this message to any of your colleagues who > recently entered the field of stellar variability and may therefore not > yet be in our mailing list or to anyone who you think might be interested > in attending the meeting. > > We look forward to seeing you in Christchurch next year! > > Don Kurtz and Karen Pollard (Co-chairs, SOC) > > > ...on behalf of the Scientific Organizing Committee: > > Don Kurtz, UK (co-chair) > Karen Pollard, New Zealand (co-chair) > Conny Aerts, Belgium > Guiseppe Bono, Italy > Joergen Christensen-Dalsgaard, Denmark > Margarida Cunha, Portugal > Gilles Fontaine, Canada > Jin-Xin Hao, China > Janusz Kaluzny, Poland > Dante Minniti, Chile > Masao Takata, Japan > George Wallerstein, USA > Patricia Whitelock, South Africa > Peter Wood, Australia > > ...and the Local Organising Committee: > > John Hearnshaw (chair), Michael Albrow, Peter Cottrell, Eddie Davis, > Carol McAlavey, Karen Pollard, Denis Sullivan, William Tobin. > > > ------------------------------------------------------------------------ > Expression of interest form to receive further correspondence > Return to: iau193@cont.canterbury.ac.nz by 1 November 2002 > ------------------------------------------------------------------------ > > IAU Colloquium 193 > Variable stars in the Local Group > > 6 - 11 July 2003, Christchurch, New Zealand > > Name: _______________________________________ > > Postal address: _______________________________________ > > _______________________________________ > > _______________________________________ > > Telephone: _______________________________________ > > FAX: _______________________________________ > > e-mail address: _______________________________________ > > Please mark one response with X: > > ____ I will definitely attend > > ____ I will probably attend > > ____ I may attend > > I would like to present a paper (if you are an invited speaker, please > fill in this part only if you wish to present an additional paper) > > ____ contributed talk > > Tentative title: > > > > ____ poster > > Tentative title: > > > > ____________________________________________________________________________