***************************************************************************** E S O W O R K S H O P on T H E R O L E O F D U S T I N T H E F O R M A T I O N O F S T A R S ****************************************************************************** Ralf Siebenmorgen Hans Ulrich K"aufl rsiebenm@iso.vilspa.esa.es hukaufl@eso.org ESA ESO Villafranca del Castillo Satellite Tracking Station Karl-Schwarzschild-Str. 2 P.O. Box 50727 E 28080 Madrid, Spain D-85748 Garching, Germany tel + 34 1 813 1366 tel + 49 89 32006 414 fax + 34 1 813 1308 fax + 49 89 32006 480 Dear Colleagues! The European Southern Observatory (ESO) is presently constructing its Very Large Telescope (VLT), an array of 4 eight meter telescopes. To keep the VLT observatory and its scientific instrumentation in phase with the evolution of astronomical research ESO is organizing selected workshops dedicated to specialized fields of current research. In this context we are happy to announce a workshop devoted to THE ROLE OF DUST IN THE FORMATION OF STARS to be held Sept. 11-14, 1995, at ESO headquarters in Garching b. M"unchen (Germany). The workshop will start on Monday Sept. 11th at 9h00 and will end on Thursday, Sept. 14th at 17h00. The objective of the workshop is to have an exchange between observers, experimentalists and theoreticians. The discussion shall encompass the status of observations and observational techniques, laboratory experiments and theoretical research with emphasis on what is needed to test predictions and to constrain models. The SCIENTIFIC ORGANIZATION of the workshop is by: - Rolf Chini and Endrik Kr"ugel, MPIfR, Bonn, Germany - Thomas Henning, MPG-AG Dust and Star Formation, Jena, Germany - John Mathis, Univ. Wisconsin, Madison, USA - Antonella Natta, Oss. Astronomico Arcetri, Italy - Jean-Loup Puget, IAS, Orsay, France - Alexander Tielens, NASA Ames, Moffet Field, USA - Nikolai Voshchinnikov, Astronomical Institute, St. Petersburg, Russia The workshop is ORGANIZED LOCALLY by: - Hans Ulrich K"aufl, ESO, Garching, Germany - Ralf Siebenmorgen, ESA, Vilafranca, Spain SEMI-FINAL PROGRAM ESO workshop The Role of Dust in the Formation of Stars To be held at ESO headquarters, Garching, Germany on Sept. 11 to 14, 1995 Sunday, Sept. 10 : ================= 18:00 - ???? Stammtisch Monday, Sept. 11 : ================== 8:30- 9:00 Registration etc. 9:00- 9:15 Official opening by R. Giacconi, ESO director General 9:15 (35+10) G. Monnet: Presentation of the VLT Project and the VLT Scientific Instruments Session 1: Present observations of YSOs 10:00 (30+5) F. Adams: The Radiative Signature of Star Formation: Spectral Evolution 10:35 (15+5) D. Leisawitz: An Overview of the COBE Infrared Datasets 10:55 Coffee-break 11:20 (15+5) D. Ward-Thompson: Submillimetre Continuum Studies of Protostars 11:40 (15+5) P. Andre: Detailed Studies of Class 0 Protostars 12:00 (25+5) J.P. Emerson: Mid-infrared Imaging of the YSO WL16: The Spatial Distribution of the Hydrocarbon Emission Features The mid-infrared PAH features in the YSOs WL16 & WL22 12:30 LUNCH 13:45 (30+5) H. Butner: The Impact of Far-Infrared Spatial Observations on Star Formation Models for Herbig Ae/Be Stars and Low Mass Stars 14:20 (15+5) P.O. Lagage: Mid IR imaging of dust around Young Stellar Objects 14:40 (15+5) Launhardt: Dust Emission from Bok Globules 15:00 COFFEE/TEA in the POSTER Gallery 16:10 (15+5) M. Hoare: Near-IR speckle observations of luminous YSOs 16:30 (15+5) T. Hayward: High Spatial Resolution Mid-Infrared Observations of Orion and other Regions of Star Formation 16:50 (15+5) N. Ageorges: High angular resolution near-infrared observations of the circumstellar environment of young stellar objects 17:10 (15+5) H.J. Staude: Dust as a tool to study the neutral outflows from luminous YSOs 17:30 (15+5) A. Zavagno: YSOs in L1641: Dust Properties Derived from Submillimeter Continuum Spectra 17:50 (15+5) T. Gledhill: Linear and Circular Imaging Polarimetry of YSOs at Near IR Wavelengths 18:15 - 19:45 Informal Reception at ESO ----------------------------------------------------- ============================================================================ Tuesday continue: Session 1: Present observations of YSOs 8:45 (35+5) P. Artymowicz: Vega Type Systems 9:25 (15+5) D. Mouillet: Dust around Main Sequence stars 9:45 (15+5) E. Pantin: Dust around beta-Pictoris: Composition and Distribution 10:05 (15+5) H.J. Walker: Silicate dust in Vega-like stars 10:25 COFFEE 10:50 (15+5) M. Gerbaldi: Are lambda Boo Stars and Vega-like Stars Related? 11:10 (15+5) H. Holweger: High-resolution spectroscopy of Lambda Bootis stars and `dusty' A stars: circumstellar gas, rotation, and accretion 11:30 (15+5) P. Saraceno: The Correlation Between Bolometric Luminosity and Millimeter Flux of the Class I Sources Exciting Outflows 11:50 (15+5) W. Schutte: Formaldehyde and Methanol Dominated Ices Towards GL 2136 Session 2: Properties of dust around YSOs 12:10 (20+5) E. Kr"ugel: Dust in Protostellar Cores 12:35 LUNCH 13:45 (20+5) A. Jones: The Dust Size Distribution and Grain Shattering in Shock Waves 14:10 (20+5) A. Tielens: The Composition of Interstellar Dust 14:35 (20+5) T. Henning: 15:00 (15+5) L. Colangeli: Simulation in the Laboratory of Cosmic Carbon Grains 15:20 COFFEE 16:00 (30+5) L. d'Hendecourt: Solid state infrared features: a diagnostic for chemical interaction between gas and grains 16:35 (15+5) M. E. Palumbo & Strazzula: Laboratory Experiments on CO and CO$_2$ ices 16:55 (15+5) P. Ehrenfreud: Infrared Properties of Isolated Water Ice 17:15 (15+5) P. Cox: Mid- and Far-Infrared Emission Bands in Carbon-rich Sources 17:35 (15+5) Y. Aikawa: Evolution of the molecular abundance in protoplanetary disks: Depletion of CO molecules} -------------------------------------------------- Wednesday, 13. Sept. : ===================== Session 3: Processing of dust in YSOs 8:30 (25+5) N Evans: The Galactic Dust Recycling Bank 9:00 (30+5) M. Greenberg: Silicate Emission in Protoplanetary Disks 9:35 (30+5) J.P. Lafon: Electrical Charging of Dust; a Review 10:10 (20+5) G. Ciolek: The Roles of Ambipolar Diffusion, Interstellar Dust, and UV Radiation in the Formation of Stars 10:35 COFFEE 11:10 (15+5) N. Berruyer: Dynamical Aspects of Dust Radiation Interaction in Flat Circumstellar Disks 11:30 (15+5) D. Currie: 3D Structure of the Bi-Polar Dust Shell of eta Carinae 11:50 (15+5) D. Puy: Primordial Molecules and Protoclouds 12:10 (15+5) J. Krelowski: On the absence of diffuse band carriers in opaque circumstellar disks 12.30 LUNCH Session 4: Models 13:40 (35+5) C. Leung: Modeling Radiation Transport in a Dusty Medium 14:20 (25+5) Steinacker: 3D Continuum Radiative Transfer 14:50 Coffee served in the POSTER Gallery 16:30 (35+5) Yorke: On the role of dust in the formation of massive stars 17:10 (25+5) Voshchinnikov: Dust shells around Herbig Ae/Be stars 17:40 (15+5) Lorenzetti: Investigating the Circumstellar Morphology of the Herbig AeBe Stars 19:30 Conference Dinner Thu : ====== 8:30 (15+5) Z. Ivezic: Infrared Classification of Young Stellar Objects 8:50 (15+5) M. Campbell: Radiative Transfer Models of Far-Infrared from W3 IRS4 and IRS5 9:10 (15+5) F. O. Clark: Observations Supporting a Conglomerate Model of Small Dust Grains 9:30 COFFEE Session 5: Dust as a catalytic agent for star formation ---------- 10:00 (30+5) T. Nakano: The Effect of Dust on the Dissipation of Magnetic Fields in Molecular Clouds 10:35 (30+5) T. Mouschovias: Role of Dust in Protostar Formation 11:10 (15+5) M. Wardle: Dusty Magnetized Protostellar Disks and the Origin of Bipolar Flows 11:30 (15+5) C. Smith: Thermal imaging of aligned grains in star-formation regions 11:50 (25+5) H. Zinnecker: Starformation in the Absence of Dust 12:20 Lunch 13:30 (15+5) Sablotny: Chemistry in Molecular Clouds without and with Dust 13:50 (15+5) Paatz & Camenzind: Winds and forbidden emission lines of T Tauri stars 14:10 (15+5) H. Wiesemeyer: Low Mass Star Formation in Globular Filaments: Evidence from Dust and Molecular Line Emission 14:30 COFFEE 15:00 (15+5) J. M. C. Rawlings: The Effects of Gas-Grain Interactions on Protostellar Line Profiles 15:20 (15+5) G. Wuchterl: Protostellar Collapse Towards Deuterium Burning 15:40 (15+5) E. G"unther: Magnetic Fields of T-Tauri Stars 16:00 (15+5) P.A. Bernasconi: Optically thick MS Evolution of still forming massive stars: first numerical results Closing : --------- 16:20 (25+x) Chr. Waelkens: Summary of Workshop waiting list: Richichi and Leinert Barsony Zubko ============================================================================= LIST OF POSTERS S. Aiello : The Response of Dust to the UV Radiation: High Density Regions no abstract C. Cervetto: Cosmic-ray Induced Charging of Dust Grains no abstract, read by Aiello G. Barbaro: Properties of dust associated with molecular clouds versus that in neutral or ionized clouds M. Barsony: IRAS HIRES Images of the Serpens Core A. Blanco: Radiation Transfer Modelling of the IR Emission from Disks around Vega-Type Stars I. Cermak: Laboratory Studies of Electric Charging of~Dust~Particles J. Chan: A Catalogue of Massive Young Stellar Objects: A Short Introduction S. Clark: Polarisation by Scattering off Dust in the Outer Envelope of YSO J.C. Correia: Compact Molecular Outflows from Young Stellar Objects in L1641 R.M. Danen: Subarcsecond 10um Imaging of Luminous Young Stellar Objects B. Dent: The Anatomy of a Resolved Protostellar Disc M. Egan: Ambipolar Diffusion and Interstellar Chemistry Efstathiou & Siebenmorgen: Models of dusty discs including transiently heated particles P. Giovanetti: Determination of the Luminosity Function of the Serpens Cloud Core from Deep V, R, I, J, H and K Images T. Giannini: Star Formation in the Vela Molecular Clouds: First Results of a Near Infrared Imaging Survey P. Hofner: High Resolution Mid-Infrared Observations of the Hot Dust in Ultracompact HII Regions C. Koempke: Gas and Dust in the S135 Star Formation Region M. Kress: Alcohols and Nitriles in Hot Cores N. Krivova: Multi Wavelength Study of HAEBE Stars with Algol-Like Minima N. Krivova: The Modelling of the IR Intensity Maps for HAEBE Stars with Algol-like Minima M. Kun: Star formation in the Cepheus Flare molecular complex S. Maddison: Simulating Dusty Gas Using SPH V. Mennella: UV IRRADIATION OF SMALL HYDROGENATED CARBON GRAINS A.B. Men'shchikov: 2-D Radiative Transfer Modeling of Embedded YSOs HL Tau and L1551 IRS 5: What is Inside? F. Motte: Size and Density Structure of Low-Mass Protostellar Envelopes T. Neckel: Two YSOs and two Herbig-Haro-jets in the PV Cephei nebula D. Nurnberger: 1.3mm dust continuum observations of young X-ray~selected stars in Ophiuchus R. Oudmaijer: Observations of young stellar objects and/or The enigmatic massive object IRC 10420 no abstract, off-topic G. Palumbo: IRAS Selected Galactic Star-Forming Regions: Water Maser Detections in Molecular Cores no abstract P. Palumbo: STARDUST: A STUDY OF THE NUCLEATION PRODUCTS IN MICROGRAVITY CONDITIONS B. Patzer: Dust Grain Processing: A new Computational Method Applied to a Protostellar Accretion Shock A. Richichi: Observation of Binaries and Envelopes in HAe/Be Stars waiting list M. Rosa: Dust and IMF properties of evolved localized star bursts in external galaxies R. Shipman: The Composition and Distribution of Dust Grains in Galactic H II Regions R. Shipman: The Effects of Clumping on Calculated Grain Properties R. Siebenmorgen: Signature of the dust composition towards Herbig--Haro sources G. Sloan: PAHs as probes of photodissociation regions in M17 and the Orion Bar R. Szczerba: Dust around post-AGB sources with 21 and 30 ${\mu}$m features M. Tapia: STAR FORMATION IN THE NORTHERN REGION OF NGC 6334 S.D. Taylor The Distribution of the Molecules CS and NH3 in Star-Forming Regions T. Teixeira: Ice Cocktails in Molecular Cloud Cores V. Toth: Triggered core formation in nearby interstellar clouds Catalogue of IRAS Loops in the IInd Galactic Quadrant E. Tommasi: Morphology of the Star Forming Region Associated with HH25-26 H.J. Walker: Searching for new Young Stars in the IRAS Point Source Catalogue W. Wegner: The shape of extinction curve in opaque circumstellar matter V. Zubko: Optical constants of amorphous carbon extracted from recent laboratory extinction measurements V. Zubko: Modelling of interstellar extinction using the method of regularisation (waiting list) ==================== end of program ===================================== The PROCEEDINGS of this meeting will be published by Springer Verlag as part of a new ESO Scientific Workshop series. Instructions for the preparation of manuscripts are included as appendix. Registered participants will automatically receive a copy of the Proceedings. There will be a REGISTRATION FEE of DM 150.00 payable at the meeting. The fee covers the cost for a copy of the proceedings, an informal reception at ESO, coffee and refreshments during the meeting and transportation between the hotels and the workshop venue. Deadline (ABSOLUTE) for manuscripts: 15 Oct. 1995 ============================================================================= ELECTRONIC ONLINE INFORMATION SERVICES All information about this workshop is available via WWW (ESO homepage) http://http.hq.eso.org/stardust.html or using the finger command finger stardust@mc6.hq.eso.org ============================================================================= APPENDIX 1 ESO Workshop on "THE ROLE OF DUST IN THE FORMATION OF STARS" INSTRUCTIONS FOR AUTHORS -------------------------- CONTRARY TO OUR PREVIOUS MAILINGS WE WILL PUBLISH THE PROCEEDINGS USING LATEX RATHER THAN TEX ! ESO has changed the form of publication of its Workshop and Conference proceedings. Future proceedings will be published by Springer in a new series with format similar to 'Lecture Notes in Physics'. NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW NEW Springer have LATEX macros to produce papers in the required format. To obtain the LATEX macro package, use anonymous ftp to ftp.hq.eso.org (134.171.40.2) and login as anonymous and change directory to /pub/esoproceedings/latex Get the following files: lamuphys.doc lamuphys.dem lamuphys.sty README_LATEX Please use these macros to format your contribution. In particular, running LATEX on the file lamuphys.doc will produce detailed instructions for preparing your document. lamuphys.dem is a sample proceedings contribution. The submission should be in paper form with all figures and tables etc. mounted and in parallel as email. Colour figures will exceptionally be accepted only if very well justified. We plan to have an object and subject index to the proceedings and therefore would appreciate if the authors could make key word suggestions. The page limits are: papers >= 30 min. (incl. discussion) 8 pages papers >= 25 min. (incl. discussion) 6 pages Contributed talks and posters 4 pages Please try to observe these limits. It is anticipated that some editorial overview will be excercised and authors may be requested to make changes to their papers. The paper copies of the manuscripts should be send to: H.U. K"aufl ESO STARDUST Karl-Schwarzschild-Str. 2 D-85748 Garching bei Muenchen Germany and the LATEX-files e-mailed to stardust@eso.org. ==================================================================== The ABSOLUTE DEADLINE for receipt of manuscripts is 15 October 1995. ==================================================================== Please contact the organizers via stardust@eso.org in the event of any questions or difficulties. In cases of urgent matters you can off course also use our personal accounts ( cstoffer@eso.org or hukaufl@eso.org ). ----------------------------------------------- VERSION August 11, 1995 ============================================================================= ELECTRONIC ONLINE INFORMATION SERVICES All information about this workshop is available via WWW (ESO homepage) http://http.hq.eso.org/stardust.html or using the finger command finger stardust@mc6.hq.eso.org ====================== EOF ===================== version August 11, 1995 ======