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[vsnet-conference 51] Fwd: IAU Colloquium 193 First Announcement
- Date: Wed, 31 Jul 2002 17:22:48 +0900
- To: Vsnet-Conference <vsnet-conference@ooruri.kusastro.kyoto-u.ac.jp>
- From: Toshihito Ishida <ishida@nhao.go.jp>
- Subject: [vsnet-conference 51] Fwd: IAU Colloquium 193 First Announcement
- Sender: owner-vsnet-conference@ooruri.kusastro.kyoto-u.ac.jp
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:
>
>
>
> ____________________________________________________________________________
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