Curriculum Vitae
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2014 Activities Report
ACTIVITIES 2014 REPORT TM2 Business Centre 34 ACTIVITIES 2014 REPORT TABLE OF CONTENTS 4 Message from the Chairman of the Board 5 Message from the President and CEO 6 Board Activities 8 2014 Strategic Planning 10 Economic Climate 13 Financial Position 14 Results of the 2014 Action Plan Saint-Laurent Campus 16 18 2008-2014 Trends 21 Real Estate Activities 23 New Resident Companies 24 Our Residents’ Achievements 28 Athletic and Social Events 30 Transportation Éco-campus Hubert Reeves 32 32 Progress Report TM2 Business Centre 34 35 2014 Year in Review 35 New Resident Companies 35 Activities and Events Health District 36 Communications Activities 38 38 Visiting Delegations 39 Advertizing and Promotion 40 Communications and Networking Events 43 International Conferences Real Estate Prospecting 46 3 MESSAGE FROM THE CHAIRMAN OF THE BOARD Paul Saint-Jacques I am delighted to report that 2014 was None of these positive results would I must also underscore the outstanding an exceptional year in many ways. have been possible without the Board’s work and results produced by our For starters, we welcomed many ongoing commitment and close President and CEO and his dedicated new residents to our Saint-Laurent cooperation with senior management. team who, despite their limited size, Campus. We also finalized several once again rose to every challenge and land sale agreements pursuant to the The Board fulfilled its governance duties met every target. strategic orientation set by our Board by taking an active role on many new of Directors a few years ago and the fronts this year, holding 20 face-to-face I invite everyone in the TM family, our sales strategy implemented by senior or video conference meetings. -
Hollenbach D CV2008.Pdf
SUMMARY CURRICULUM VITA DAVID JOHN HOLLENBACH Education: PhD., Theoretical Physics, Cornell University, 1969 Present Area of Research: Theoretical astrophysics, infrared astronomy, interstellar medium, star formation, astrochemistry, astrobiology Professional Activities: Senior member of American Astronomical Society, Senior member of International Astronomical Union, Study Scientist Large Deployable Telescope (LDR) Project (1980-84), Member of NASA Astronomy and Relativity Management Operation Working Group (ARMOWG) (1985-88), Scientific Organizing Committee for IAU Symposium 120, “Astrochemistry” (1984-85), Scientific Organizing Committee for Summer Schools on "Interstellar Processes”, The Interstellar Medium of Galaxies", and "The Evolution of Galaxies and Their Environment" (1985-1992), Director (PI) of the Center for Star Formation Studies, a consortium of NASA-Ames, UC Berkeley, and UC Santa Cruz Theoretical Astrophysicists funded by the NASA Theory Program (1985-2002), Member of the Executive Committee for the Space Sciences Laboratory, UC Berkeley (1985-1995), Co-Investigator on the Submillimeter Wave Astronomical Satellite (SWAS)(1988-present), Member of the Infrared Panel of the National Academy of Sciences Astronomy Astrophysics Survey Committee(1988-1990), Member of the ISO Short Wavelength Spectrometer Team (1990-2000), Member of the Stratospheric Observatory for Infrared Astronomy (SOFIA) Science Working Group (1990-1995), Member of the Submillimeter Science Working Group (1985-1995), Member of Executive Council of the American -
Book of Abstracts
THE PHYSICS AND CHEMISTRY OF THE INTERSTELLAR MEDIUM Celebrating the first 40 years of Alexander Tielens' contribution to Science Book of Abstracts Palais des Papes - Avignon - France 2-6 September 2019 CONFERENCE PROGRAM Monday 2 September 2019 Time Speaker 10:00 Registration 13:00 Registration & Welcome Coffee 13:30 Welcome Speech C. Ceccarelli Opening Talks 13:40 PhD years H. Habing 13:55 Xander Tielens and his contributions to understanding the D. Hollenbach ISM The Dust Life Cycle 14:20 Review: The dust cycle in galaxies: from stardust to planets R. Waters and back 14:55 The properties of silicates in the interstellar medium S. Zeegers 15:10 3D map of the dust distribution towards the Orion-Eridanus S. Kh. Rezaei superbubble with Gaia DR2 15:25 Invited Talk: Understanding interstellar dust from polariza- F. Boulanger tion observations 15:50 Coffee break 16:20 Review: The life cycle of dust in galaxies M. Meixner 16:55 Dust grain size distribution across the disc of spiral galaxies M. Relano 17:10 Investigating interstellar dust in local group galaxies with G. Clayton new UV extinction curves 17:25 Invited Talk: The PROduction of Dust In GalaxIES C. Kemper (PRODIGIES) 17:50 Unravelling dust nucleation in astrophysical media using a L. Decin self-consistent, non steady-state, non-equilibrium polymer nucleation model for AGB stellar winds 19:00 Dining Cocktail Tuesday 3 September 2019 08:15 Registration PDRs 09:00 Review: The atomic to molecular hydrogen transition: a E. Roueff major step in the understanding of PDRs 09:35 Invited Talk: The Orion Bar: from ALMA images to new J. -
Physical Processes in the Interstellar Medium
Physical Processes in the Interstellar Medium Ralf S. Klessen and Simon C. O. Glover Abstract Interstellar space is filled with a dilute mixture of charged particles, atoms, molecules and dust grains, called the interstellar medium (ISM). Understand- ing its physical properties and dynamical behavior is of pivotal importance to many areas of astronomy and astrophysics. Galaxy formation and evolu- tion, the formation of stars, cosmic nucleosynthesis, the origin of large com- plex, prebiotic molecules and the abundance, structure and growth of dust grains which constitute the fundamental building blocks of planets, all these processes are intimately coupled to the physics of the interstellar medium. However, despite its importance, its structure and evolution is still not fully understood. Observations reveal that the interstellar medium is highly tur- bulent, consists of different chemical phases, and is characterized by complex structure on all resolvable spatial and temporal scales. Our current numerical and theoretical models describe it as a strongly coupled system that is far from equilibrium and where the different components are intricately linked to- gether by complex feedback loops. Describing the interstellar medium is truly a multi-scale and multi-physics problem. In these lecture notes we introduce the microphysics necessary to better understand the interstellar medium. We review the relations between large-scale and small-scale dynamics, we con- sider turbulence as one of the key drivers of galactic evolution, and we review the physical processes that lead to the formation of dense molecular clouds and that govern stellar birth in their interior. Universität Heidelberg, Zentrum für Astronomie, Institut für Theoretische Astrophysik, Albert-Ueberle-Straße 2, 69120 Heidelberg, Germany e-mail: [email protected], [email protected] 1 Contents Physical Processes in the Interstellar Medium ............... -
Discoveries of Mass Independent Isotope Effects in the Solar System: Past, Present and Future Mark H
Reviews in Mineralogy & Geochemistry Vol. 86 pp. 35–95, 2021 2 Copyright © Mineralogical Society of America Discoveries of Mass Independent Isotope Effects in the Solar System: Past, Present and Future Mark H. Thiemens Department of Chemistry and Biochemistry University of California San Diego La Jolla, California 92093 USA [email protected] Mang Lin State Key Laboratory of Isotope Geochemistry Guangzhou Institute of Geochemistry, Chinese Academy of Sciences Guangzhou, Guangdong 510640 China University of Chinese Academy of Sciences Beijing 100049 China [email protected] THE BEGINNING OF ISOTOPES Discovery and chemical physics The history of the discovery of stable isotopes and later, their influence of chemical and physical phenomena originates in the 19th century with discovery of radioactivity by Becquerel in 1896 (Becquerel 1896a–g). The discovery catalyzed a range of studies in physics to develop an understanding of the nucleus and the properties influencing its stability and instability that give rise to various decay modes and associated energies. Rutherford and Soddy (1903) later suggested that radioactive change from different types of decay are linked to chemical change. Soddy later found that this is a general phenomenon and radioactive decay of different energies and types are linked to the same element. Soddy (1913) in his paper on intra-atomic charge pinpointed the observations as requiring the observations of the simultaneous character of chemical change from the same position in the periodic chart with radiative emissions required it to be of the same element (same proton number) but differing atomic weight. This is only energetically accommodated by a change in neutrons and it was this paper that the name “isotope” emerges. -
Modelling Ionised and Photodissociated Regions
Modelling ionised and photodissociated regions Magda Vasta Thesis submitted for the Degree of Doctor of Philosophy of University College London Department of Physics & Astronomy UNIVERSITY COLLEGE LONDON March 2010 I, Magda Vasta, confirm that the work presented in this thesis is my own. Where information has been derived from other sources, I confirm that this has been indicated in the thesis. To my parents, my brother and my husband, who always supported and encouraged me no matter what. I tell people I am too stupid to know what is impossible. I have ridiculously large dreams, and half the time they come true. — Thomas D. ACKNOWLEDGEMENTS Some people come into our lives and quickly go. Some stay for a while and leave footprints on our hearts. And we are never, ever the same. I made it, I still cannot believe it, but I finally made it. However, it would have been almost impossible to reach this target without the constant scientific support from some people. My first big THANKS go to my supervisor Serena Viti. Thanks for being the supportive person you are, for giving me the possibility to be independent in my research, but being always present when I needed you. Thanks for all the times that you did not talk to me in Italian, for encouraging me to not give up and for being the lovely person you are. Thanks to Mike Barlow for the amazing scientific suggestions and for tolerating ALL my silly questions (most of them grammatically incorrect!). Thanks to Barbara Ercolano for her patience when answering my emails “HELP, PLEASE!!” about MOCASSIN. -
Bibliothèque Et Archives Canada
National Library Bibliothèque nationale 1+1 of Canada du Canada Acquisitions and Direction des acquisitions et Bibliographie Services Branch des services bibliographiques 395 Wellington Street 395. rue Wellington Ottawa. Ontario O"aoo (Onlaoo) K1AON4 K1AON4 NOTICE AVIS The quality of this microform is La qualité de cette microforme heavily dependent upon the dépend grandement de la qualité quality of the original thesis de la thèse soumise au submitted for microfilming. microfilmage. Nous avons tout Every effort has been made to fait pour assurer une qualité ensure the highest quality of supérieure de reproduction. reproduction possible. If pages are missing, contact the S'il manque des pages, veuillez university which granted the communiquer avec l'université degree. qui a conféré le grade. Some pages may have indistinct La qualité d'impression de print especially if the original certaines pages peut laisser à . pages were typed with a poor désirer, surtout si les pages typewriter ribbon or if the originales ont été university sent us an inferior dactylographiées à l'aide d'un photocopy. ruban usé ou si l'université nous a fait parvenir une photocopie de qualité inférieure. Reproduction in full or in part of La reproduction, même partielle, this microform is governed by de cette m!croforme est soumise the Canadian Copyright Act, à la Loi canadienne sur le droit R.S.C. 1970, c. C-30, and d'auteur, SRC 1970, c. C-30, et subsequent amendments. ses amandements subséquents. Canada • THE ORIGINS AND EMERGENCE OF QUEBEC'S ENVIRONMENTAL MOVEMENT: 1970 - 1985 JANE E. BARR Geography Department McGiII University, Montreal May, 1995 A thesis submitted to the Faculty of Graduate Studies and Research in partial fulfilment of • the requirements of the degree of Master of Arts, 1995 ©, Jane E. -
D C B Whittet.Pdf
Dust in the Galactic Environment Second Edition Series in Astronomy and Astrophysics Series Editors: M Birkinshaw, University of Bristol, UK M Elvis, Harvard–Smithsonian Center for Astrophysics, USA J Silk, University of Oxford, UK The Series in Astronomy and Astrophysics includes books on all aspects of theoretical and experimental astronomy and astrophysics. Books in the series range in level from textbooks and handbooks to more advanced expositions of current research. Other books in the series An Introduction to the Science of Cosmology D J Raine and E G Thomas The Origin and Evolution of the Solar System M M Woolfson The Physics of the Interstellar Medium J E Dyson and D A Williams Dust and Chemistry in Astronomy T J Millar and D A Williams (eds) Observational Astrophysics R E White (ed) Stellar Astrophysics R J Tayler (ed) Forthcoming titles The Physics of Interstellar Dust EKr¨ugel Very High Energy Gamma Ray Astronomy T Weekes Dark Sky, Dark Matter P Wesson and J Overduin Series in Astronomy and Astrophysics Dust in the Galactic Environment Second Edition D C B Whittet Professor of Physics, Rensselaer Polytechnic Institute, Troy, New York, USA Institute of Physics Publishing Bristol and Philadelphia c IOP Publishing Ltd 2003 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without the prior permission of the publisher. Multiple copying is permitted in accordance with the terms of licences issued by the Copyright Licensing Agency under the terms of its agreement with Universities UK (UUK). -
Are the Carriers of Diffuse Interstellar Bands and Extended Red Emission
MNRAS 000,1{13 (2020) Preprint 20 January 2020 Compiled using MNRAS LATEX style file v3.0 Are the Carriers of Diffuse Interstellar Bands and Extended Red Emission the same? Thomas S. -Y. Lai1?, Adolf N.Witt1, Carlos Alvarez2, Jan Cami3;4;5 1Ritter Astrophysical Research Center, University of Toledo, Toledo, OH 43606, USA 2W. M. Keck Observatory, 65-1120 Mamalahoa Hwy., Kamuela, HI 96743-8431, USA 3Department of Physics and Astronomy, The University of Western Ontario, London, ON N6A 3K7, Canada 4Institute for Earth and Space Exploration, The University of Western Ontario, London, ON N6A 3K7, Canada 5SETI Institute, 189 Bernardo Avenue, Suite 100, Mountain View, CA 94043, USA Accepted 2020 January 13. Received 2019 December 24; in original form 2019 July 8. ABSTRACT We report the first spectroscopic observations of a background star seen through the region between the ionization front and the dissociation front of the nebula IC 63. This photodissociation region (PDR) exhibits intense extended red emission (ERE) attributed to fluorescence by large molecules/ions. We detected strong diffuse inter- stellar bands (DIB) in the stellar spectrum, including an exceptionally strong and broad DIB at λ4428. The detection of strong DIBs in association with ERE could be consistent with the suggestion that the carriers of DIBs and ERE are identical. The likely ERE process is recurrent fluorescence, enabled by inverse internal conversions from highly excited vibrational levels of the ground state to low-lying electronic states with subsequent transitions to ground. This provides a path to rapid radiative cooling for molecules/molecular ions, greatly enhancing their ability to survive in a strongly irradiated environment. -
Geographical Distribution of the Italian Astronomical Observatories
Figure 25.1: Geographical distribution of the Italian Astronomical Observatories 226 25. Italian Astronomical Observatories and their Historical Instruments Collections Ileana Chinnici (Palermo, Italy) 25.1 A Brief Historical Introduction made by famous instruments-makers of that time, such as Ramsden, Short, Sisson, etc. while the typical equip- Italy has a high number of astronomical observatories ment of an Italian observatory in the middle of the 19th in comparison with its territorial extension. This is due century consisted of astronomical instruments made by to historical reasons, as Italy results from a political Reichenbach, Fraunhofer, Repsold, Merz and others. process of unification and annexation of several small The ancient observatories, built upon towers or states into which the country was divided – a process palaces in the middle of the cities, have mostly preserved (the Risorgimento) which was carried out mainly around their original building and their historical architecture; th the half of 19 century. a special mention is to be deserved to the Naples Obser- The first “institutional” Observatories in Italy were vatory, located on the hill of the Capodimonte: it was th established in the 18 century, as in the majority of the first architectural complex in Italy specially planned the other European nations. At that time, Italy was and built to be an astronomical observatory; it dates composed by seven states and since 1711 to 1819 each back to 1819, thus preceding the Pulkovo Observatory, of these states established one or two Observatories in established in 1839, which will serve later as architec- its territory. tural model for many observatories all over the world. -
Page 1 of 5 ARIEL FENSTER OFFICE ADDRESS Mcgill University, Office for Science and Society 801 Sherbrooke St West, Montreal, Qu
ARIEL FENSTER OFFICE ADDRESS McGill University, Office for Science and Society 801 Sherbrooke St West, Montreal, Quebec H3A 0B8 Tel: (514) 398-2618 email: [email protected] EDUCATION Degree University Subject Year Licence ès Sciences (B.Sc.) Paris Mathematics, Physics & Chemistry 1966 Diplôme d'Études Paris Theoretical and Physical Chemistry 1967 Approfondies (M.Sc.) Ph.D. McGill Physical and Inorganic Chemistry 1973 AFFILIATIONS Chemical Institute of Canada American Chemical Society Quebec Association of Science Teachers AWARDS Polysar Award for Outstanding Chemistry Teaching presented by the Chemical Institute of Canada, 1982 Catalyst Award for Excellence in Chemistry Teaching presented by the US Chemical Manufacturers Association, 1989 C3 Award for Outstanding Contribution to Chemical Education presented by College Chemistry Canada (Inaugural Award), 1990 McNeil Medal for the Public Awareness of Science presented by the Royal Society of Canada, (Inaugural Shared Award with Drs. Harpp and Schwarcz), 1992 Beppo Award for Communicating Science to the Public, presented by the Conseil de développement du loisir scientifique du Québec", (Shared Award with Drs. Harpp and Schwarcz), 1993 Raymond Gervais Award for Exceptional Contributions to Science Education, presented by the Quebec Association of Science Teachers, 1999 Michael Smith Award for the Promotion of Science in Canada, presented by the Natural Sciences and Engineering Research Council of Canada, 2005 Faculty Award for Excellence in Alumni Activities, presented by the McGill -
1 the Founding of Arcetri Observatory in Florence
THE FOUNDING OF ARCETRI OBSERVATORY IN FLORENCE Simone Bianchi INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi, 5, 50125, Florence, Italy [email protected] Abstract: The first idea of establishing a public astronomical observatory in Florence, Capital of the Grand Duchy of Tuscany, dates to the mid of the 18th century. Initially, the use of a low building on a high ground was proposed, and the hill of Arcetri suggested as a proper location. At the end of the century, the Florence Observatory - or Specola - was built instead on a tower at the same level as the city’s centre. As soon as astronomers started to use this observatory, they recognized all its flaws and struggled to search for a better location. Giovanni Battista Donati, director of the Specola of Florence from the eve of the Italian Unification in 1859, finally succeeded in creating a new observatory: first, he obtained funds from the Parliament of the Kingdom of Italy to build an equatorial mount for the Amici 28-cm refractor, which could not be installed conveniently in the tower of the Specola; then, he went through the process of selecting a proper site, seeking funds and finally building Arcetri Observatory. Although Donati was a pioneer of spectroscopy and astrophysics, his intent was to establish a modern observatory for classical astronomy, as the Italian peninsula did not have a national observatory like those located in many foreign capitals – Florence was the capital of the Kingdom of Italy from 1865 to 1871. To promote the project, Donati made use of writings by one of the most authoritative European astronomers, Otto Wilhelm Struve.