MPIA Workshop on

MODES OF STAR FORMATION
and the Origin of Field Star Populations



Date:        October 9 to 13, 2000
Venue:      Max Planck Institute for Astronomy, Heidelberg, Germany
Sponsor:   Max Planck Society
Organizer:    Eva K. Grebel




Name

Affiliation

Title of talk or poster
Tom Abel Harvard Smithsonian Center for Astrophysics, Cambridge, USA The Formation of the First Star in the Universe
João Alves European Southern Observatory, Garching, Germany Lessons from the Simplest Mode of Star Formation
Holger Baumgardt University of Edinburgh, Edinburgh, UK Enrichment of the stellar halo by disrupted globular clusters
Raoul Behrend Geneva Observatory, Sauverny, Switzerland  
Christian Boily Astronomisches Recheninstitut, Heidelberg, Germany The dynamics of mass loss during the formation of open star clusters
Wolfgang Brandner Institute for Astronomy, University of Hawaii, USA Resolved Giant HII Regions: Past and Present Star Formation Properties of NGC 3603 and 30 Doradus
Anthony Brown European Southern Observatory, Garching, Germany Evolution from OB associations and moving groups to field populations
Andi Burkert Max-Planck-Institut für Astronomie, Heidelberg, Germany Star Formation in Turbulent Molecular Clouds
Roberto Capuzzo-Dolcetta Ist. Astronomico, Universitá La Sapienza, Rome, Italy Galactic nuclear activity induced by globular cluster merging
Giovanni Carraro Universitá di Padova, Italy Dwarf Spheroidal Galaxies: Structures, Star Formation and Color-Magnitude Diagrams
Chris Conselice University of Wisconsin, Madison, USA Starburst Galaxies at Low and High Redshift
Raúl de la Fuente Marcos Universidad Complutense de Madrid, Spain 1. Ghostly Open Clusters
2. Dynamics of Brown Dwarfs in Open Clusters
3. Modification of Planetary Orbits in Star Clusters
Serge Demers Université de Montréal, Canada The Young Inter-Cloud Population: More Than 5 kpc from the Nearest Site of Current Star Formation
Andy Dolphin NOAO, Tucson, USA Massive Clusters in Spiral Galaxies
Sona Ehlerová Astronomical Institute, Prague, Czech Republic Star formation in expanding shells
Bruce Elmegreen IBM Research Division, Yorktown Heights, USA A Universality to Star Formation in all Galaxy Types
Sofia Feltzing Lund Observatory, Lund, Sweden 1. The low-mass IMF as a function of the environment - deep star counts in the dSph galaxy Ursa Minor
2. Age-metallicity relation in the solar neighbourhood - or lack thereof
Andrea Ferrara Osservatorio Astrofisico Arcetri, Firenze, Italy The Role of Stellar Feedback in the Evolution of Dwarf Galaxies
Don Figer STScI and JHU, Baltimore, USA Starburst Clusters in Galactic Nuclei
Burkhard Fuchs Astronomisches Rechen-Institut, Heidelberg, Germany Implications of modes of star formation for the overall dynamics of galactic disks
Yasuo Fukui Department of Astrophysics, Nagoya University, Japan Molecular Clouds in the Local Group
Jay Gallagher University of Wisconsin, Madison, USA Modes of Star Formation in Low-Mass Disk Galaxies
Reinhard Genzel MPI für extraterrestrische Physik, Garching, Germany  
David Gittins Institute of Astronomy, Cambridge, UK Star Formation on a Crossing Time?
Dimitrios Gouliermis Sternwarte der Universität Bonn, Germany Stellar content of three LH associations East of LMC 4 and their Field in the Large Magellanic Cloud
Eva Grebel Max-Planck-Institut für Astronomie, Heidelberg, Germany Modes of Star Formation in Dwarf Spheroidal Galaxies
Daniel-Rolf Harbeck Max-Planck-Institut für Astronomie, Heidelberg, Germany Deep wide-field imaging of the Sextans dSph Galaxy
Jason Harris Univ. of California, Santa Cruz, USA The Star Formation History of the Small Magellanic Cloud
Fabian Heitsch Max-Planck-Institut für Astronomie, Heidelberg, Germany Alfvén-wave Driven Turbulence in Molecular Clouds
Thomas Henning Astrophysikalisches Institut und Universitätssternwarte, Jena, Germany How to Form Massive Stars?
Gerhard Hensler University of Kiel, Germany Star Formation in Dwarf Irregular Galaxies: From Self-regulation to Starbursts
Paul Hodge University of Washington, Seattle, USA Modes of Star Formation in Spiral Galaxies
Johan Holmberg Lund University, Lund, Sweden Old moving groups
Deidre Hunter Lowell Observatory, Flagstaff, USA Star-forming regions in irregular galaxies
Rachel Johnson Institute of Astronomy, Cambridge, UK Nuclear star formation in nearby galaxies
Guinevere Kaufmann Max-Planck-Institut für Astrophysik, Garching, Germany  
Rainer Köhler Max-Planck-Institut für Astronomie, Heidelberg, Germany Multiplicity of T Tauri Stars in Different Star Forming Regions
Joachim Krautter Landessternwarte, Heidelberg, Germany The Lupus star forming region - a paradigm for low-mass star formation
Pavel Kroupa Institut für Theoretische Astrophysik, Heidelberg, Germany 1. The formation of bound star clusters
2. On the variation of the IMF
Stan Kurtz Universidad Nacional Autónoma de México, Mexico Spiral-Density-Wave Induced Star Formation at High Galactic Latitudes
Charles Lada Smithsonian Astrophysical Observatory, Cambridge, USA The Nature of Embedded Clusters: Insights into the IMF and the Frequency of Planetary Systems in the Galaxy
Henny Lamers Astronomical Institute, Utrecht University, The Netherlands The formation of massive stars in the Bulge of M51: evidence for a different mode of star-formation?
Bernd Lang Max-Planck-Institut für Astronomie, Heidelberg, Germany  
Richard Larson Yale University, New Haven, USA Conference Summary
Sebastiano Ligori Max-Planck-Institut für Astronomie, Heidelberg, Germany  
Ute Lisenfeld IRAM, Granada, Spain Star formation in Tidal Dwarf Galaxies
Kevin Luhman Harvard-Smithsonian Center for Astrophysics, Cambridge, USA The Initial Mass Function of Stars and Brown Dwarfs: A Comparison Among Different Galactic Populations
Mordecai Mac Low American Museum of Natural History, New York, USA Isolated vs. Clustered Star Formation
Steven Majewski University of Virginia, Charlottesville, USA Accretion of Satellite Galaxies by the Milky Way
Diego Mardones Universidad de Chile, Santiago, Chile Spatial and Velocity Structure of Inward Motions Around Nearby Protostars
André Moitinho de Almeida Observatorio Astronomico Nacional, Ensenada, Mexico Spatial Structure and Star Formation in the Galactic Disk: Open Cluster Data
Thorsten Naab Max-Planck-Institut für Astronomie, Heidelberg, Germany  
Michael Odenkirchen Max-Planck-Institut für Astronomie, Heidelberg, Germany Detection of the Tidal Tails of the Globular Cluster Pal 5 with SDSS Commissioning Data
Joel Parker Southwest Research Institute, Boulder, USA  
Genevieve Parmentier Institute of Astrophysics and Geophysics, Liege, Belgium Evidence for a self- enrichment process in galactic halo globular clusters
Monika Petr Max-Planck-Institut für Radioastronomie, Bonn, Germany Isolated Young Binary Stars Near Star-Forming Regions
Thomas Preibisch Max-Planck-Institut für Radioastronomie, Bonn, Germany Triggered Star Formation in the Sco OB2 Association
Massimo Robberto STScI, Baltimore, USA The Orion Nebula Cluster at Mid-IR Wavelengths
Helio Rocha-Printo Instituto Astronomico e Geofisico, Sao Paulo, Brazil The Chemical Enrichment and Star Formation History in the Milky Way Disk
Michael Smith Armagh Observatory, Armagh, UK Triggering Stars with Protostars
Andrea Stolte Max-Planck-Institut für Astronomie, Heidelberg, Germany Constraints on the Sagittarius Dwarf Galaxy's Tidal Stream
Yu-Nung Su Graduate Institute of Astronomy, National Central University, Taiwan Dust continuum and Molecular Line Observations of Massive Protostars and Super- Ultracompact HII Regions
Linda Tacconi MPI für extraterrestrische Physik, Garching, Germany Star Formation in Merging Galaxies
Kengo Tachihara MPI für extraterrestrische Physik, Garching, Germany Statistical study of nearby dense cores and their modes of star formation
Leonardo Testi Osservatorio Astrofisico di Arcetri, Italy Star Formation in Clusters: Subclustering, Cloud Fragmentation and the Origin of the Stellar IMF
Liese van Zee Dominion Astrophysical Observatory, Victoria, Canada Comparison of Star Formation Modes in Normal Dwarf Irregulars and BCDs
Alessandro Vicari Ist. Astronomico, Universitá La Sapienza, Rome, Italy Application of an objective method of identification of young star groupings in spiral galaxies
Mareike Ziegler Max-Planck-Institut für Astronomie, Heidelberg, Germany The Velocity Structure of Turbulent Molecular Cloud Cores
Hans Zinnecker Astrophysikalisches Institut Potsdam, Germany The binary mode of star formation



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Eva K. Grebel