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The Star Clusters Young & Old Newsletter

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The Star Clusters Young & Old Newsletter SCYON The Star Clusters Young & Old Newsletter edited by Holger Baumgardt, Ernst Paunzen and Pavel Kroupa SCYON can be found at URL: http://astro.u-strasbg.fr/scyon SCYONIssueNo.31 11December2006 EDITORIAL Here is the 31st issue of the SCYON newsletter. The current issue contains 35 abstracts, an an- nouncement for a new, parallel N-body code and announcements for conferences in Italy, Germany and Armenia. It also contains job advertisements for postdoctoral and tenure track positions from Rochester Institute of Technology. We wish everybody a merry holiday season and a happy new year 2007 and thank those who sent us their contributions. Holger Baumgardt, Ernst Paunzen and Pavel Kroupa ................................................... ................................................. CONTENTS Editorial .......................................... ...............................................1 SCYON policy ........................................ ...........................................2 Mirror sites ........................................ ..............................................2 Abstract from/submitted to REFEREED JOURNALS ........... ................................3 1. Star Forming Regions ............................... ........................................3 2. Embedded Clusters................................. .........................................7 3. Galactic Center Clusters........................... ..........................................9 4. Galactic Open Clusters............................. ........................................10 5. Galactic Globular Clusters ......................... ........................................14 6. Extragalactic Clusters............................ ..........................................20 7. Dynamical evolution - Simulations. .......................................24 8. Miscellaneous.................................... ..........................................30 Abstracts of CONFERENCE PROCEEDINGS ................... ...............................31 Ph.D. (dissertation) summaries ....................... ...........................................38 Conference / announcements........................... ..........................................39 Jobs ............................................... .............................................46 2 SCYON POLICY The SCYON Newsletter publishes abstracts from any area in astronomy which are relevant to research on star clusters. We welcome all contributions. Topics to be covered include 1. Abstracts from refereed articles 2. Abstracts from conference proceedings 3. PhD summaries 4. General announcements : Conferences, new databases, and the likes. Concerning possible infringements to copyright laws, we understand that the authors themselves are taking responsibility for the material they send us. We make no claim whatsoever to owning the material that is posted at our url or circulated by email. The newsletter SCYON is a free service. It does not substitute for our personal opinions, nor does it reflect in any way the views of our respective institutes of affiliations. SCYON will be published initially once every two months. If the number of contributions justi- fies monthly installments, we will move toward more frequent issues in order to keep the newsletter relatively short, manageable for us, and up-to-date. Conference and journal abstracts can be submitted at any time either by web download, or failing this, we also accept abstracts typeset using the latest latex abstract template (available from the SCYON webpage). We much prefer contributors to use the direct download form, since it is mostly automated. Abstracts will normally appear on the website as soon as they are submitted to us. Other contributions, such as PhD summaries, should be sent to us using the LaTeX template. Please do not submit postscript files, nor encoded abstracts as e-mail attachments. All abstracts/contributions will be processed, but we reserve the right to not post abstracts sub- mitted in the wrong format or which do not compile. If you experience any sort of problems accessing the web site, or with the LaTeX template, please write to us at [email protected]. A “Call for abstracts” is sent out approximately one week before the next issue of the newsletter is finalised. This call contains the deadline for abstract submissions for that coming issue and the LaTeX abstract template. Depending on circumstances, the editors might actively solicit contributions, usually those spotted on a preprint server, but they do not publish abstracts without the author’s consent. We implicitly encourage further dissemination of the letter to institutes and astronomers who may benefit from it. The editors SCYON Mirrors The official Scyon mirror site in Australia is hosted at the Centre for Astrophysics & Supercomputing of the University of Swinburne by Duncan Forbes and his team : http://astronomy.swin.edu.au/scyon/) ABSTRACTS FROM REFEREED JOURNALS 3 1. Star Forming Regions Current Star Formation in the Perseus Molecular Cloud: Constraints from Unbiased Submillimeter and Mid-Infrared Surveys Jes K. Jørgensen (1), Doug Johnstone (2,3), Helen Kirk (3,2), & Philip C. Myers (1) (1) Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS42, Cambridge, MA 02138, USA, (2) Herzberg Institute of Astrophysics, National Research Council of Canada, 5071 West Saanich Road, Victoria, BC V9E 2E7, Canada, (3) Department of Physics & Astronomy, University of Victoria, Victoria, BC, V8P 1A1, Canada We present a census of the population of deeply embedded young stellar objects (YSOs) in the Perseus molecular cloud complex based on a combination of Spitzer Space Telescope mid-infrared data from the “Cores to Disks” (c2d) legacy team and JCMT/SCUBA submillimeter maps from the COMPLETE team. The mid-infrared sources detected at 24 µm and having [3.6] − [4.5] > 1 are located close to the center of the SCUBA cores, typically within 15′′ of their peaks. The narrowness of the spatial distribution of mid-infrared sources around the peaks of the SCUBA cores suggests that no significant dispersal of the newly formed YSOs has occurred. This argues against the suggestion that motions of protostars regulate the time scales over which significant (Bondi-Hoyle) accretion can occur. The YSOs are found to have red [3.6] − [4.5] and [8.0] − [24] colors, but not comparable red [5.8]−[8.0] colors. The most deeply embedded YSOs are found in regions with high extinction, AV ≥ 5, similar to the extinction threshold observed for the SCUBA cores. All the SCUBA cores with high concentrations have embedded YSOs, but not all cores with low concentrations are starless. From the above considerations a relatively unbiased sample of 49 deeply embedded YSOs is constructed. Embedded YSOs are found in 40 of the 72 SCUBA cores with only three cores harboring multiple embedded YSOs within 15′′. The equal number of SCUBA cores with and without embedded YSOs suggests that the time scale for the evolution through the dense prestellar stages, where the cores are recognized in the submillimeter maps and have central densities of 5 × 104 − 1 × 105∼cm−3, is similar to the time scale for the embedded protostellar stages. The current star formation efficiency of cores is estimated to be approximately 10–15%. In contrast, the star formation efficiency averaged over the cloud life time and compared to the total cloud mass is only a few percent, reflecting also the efficiency in assembling cloud material into the dense cores actually forming stars. To appear in : (astro-ph/0610381) For preprints, contact [email protected] Also available from the URL http://arxiv.org/abs/astro-ph/0610381 or by anonymous ftp at ................................................... ................................................. ABSTRACTS FROM REFEREED JOURNALS 4 A kinematic study of the Taurus-Auriga T association Claude Bertout & Francoise Genova Institut d’Astrophysique de Paris Observatoire de Strasbourg Aims: This is the first paper in a series dedicated to investigating the kinematic properties of nearby associations of young stellar objects. Here we study the Taurus-Auriga association, with the primary objective of deriving kinematic parallaxes for individual members of this low-mass star-forming region. Methods: We took advantage of a recently published catalog of proper motions for pre-main sequence stars, which we supplemented with radial velocities from various sources found in the CDS databases. We searched for stars of the Taurus-Auriga region that share the same space velocity, using a modified convergent point method that we tested with extensive Monte Carlo simulations. Results: Among the sample of 217 Taurus-Auriga stars with known proper motions, we identify 94 pre-main sequence stars that are probable members of the same moving group and several additional candidates whose pre-main sequence evolutionary status needs to be confirmed. We derive individual parallaxes for the 67 moving group members with known radial velocities and give tentative parallaxes for other members based on the average spatial velocity of the group. The Hertzsprung-Russell diagram for the moving group members and a discussion of their masses and ages are presented in a companion paper. Accepted by : Astronomy & Astrophysics For preprints, contact Also available from the URL http://arxiv.org/abs/astro-ph/0610506 or by anonymous ftp at ftp:// ................................................... ................................................
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