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================================================================================ First Announcement: GAS AND GALAXY EVOLUTION: A Conference in Honor of the 20th Anniversary of the VLA Socorro, NM USA 21-24 May 2000 ================================================================================ In celebration of 20 years of VLA observations, NRAO and New Mexico Tech are jointly sponsoring a conference in Socorro, New Mexico, on 21-24 May 2000. The theme is the role of gas in galaxy evolution, concentrating on the interplay between galaxies and their environments, with some emphasis on HI imaging. Questions we hope to address include: What are the residual signatures of the formation process around galaxies? Do galaxies evolve along the Hubble sequence? If so, how, and in what direction? Do mergers really convert spirals to ellipticals? Can continuing accretion `grow' dynamically-cold disks into the present? What can we learn about the history and fate of galaxies from the structure of their gaseous envelopes? We would like to confront the vast range of current observations with theoretical predictions and interpretations, and to map out new directions for the future. The conference will conclude with a celebration of the twentieth anniversary of the VLA, held at the VLA site. The registration fee will be around $175, which includes a book of the conference proceedings and all-you-can-eat sopaipillas. We especially encourage recent graduates to attend! Current information on the meeting will be maintained on the Web at http://www.nrao.edu/vla2000 Please pre-register using the Web form accessible from that page (preferably), or the ASCII form at the bottom of this email, if you would like to be kept on this mailing list. We anticipate a second mailing in mid-November. A preliminary list of topics is as follows: I. Gas content as a function of z, in the context of large scale structure II. Galaxy formation and High redshift Galaxies III. Nearby Galaxies in (Trans)formation IV. Nearby Galaxies A. Stable long lived structures or continually evolving? B. Dark matter aspects of HI work V. The Influence of Galaxies on Their Surroundings VI. Environmental Effects on the Gas in Galaxies VII. Outstanding Questions and Future Instruments VIII. Summary The SOC consists of Jacqueline van Gorkom, chair (Columbia Univ.) James Binney (Oxford) Julianne Dalcanton (Univ. of Washington) Ron Ekers (CSIRO) Ken Freeman (ANU) John Hibbard (NRAO/CV) Michael Rupen (NRAO/Socorro) Renzo Sancisi (Bologna) Francois Schweizer (Carnegie Institute) Linda Sparke (Univ. of Wisconsin) David Westpfahl (New Mexico Tech) Ann Zabludoff (Univ. of Arizona) We look forward to seeing you! -- Michael Rupen, on behalf of the Scientific Organizing Committee =========================<-- D E T A C H H E R E -->========================== IF YOU WISH TO BE KEPT ON THIS MAILING LIST, either (1) fill in the Web form, accessible from http://www.nrao.edu/vla2000 or (2) fill out the following and email to vla2000@aoc.nrao.edu Last name: ______________________________________________ First name: ______________________________________________ Institution: ______________________________________________ Further information should be sent via (check one): ___ email email address: _______________ ___ ordinary mail Mailing address: _____________________________________________________ _____________________________________________________ _____________________________________________________ _____________________________________________________ _____________________________________________________ ___ fax fax number: ___________________ Participation: ___ I would like to give a talk (give title below) ___ I would like to present a poster (give title below) Preliminary title: ________________________________________________________ ________________________________________________________ ________________________________________________________ ___ I will definitely attend _X_ I wish to be kept on the mailing list ================================================================================
Last modified 25 October 1999
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