It is now known that most, if not all, of the stars in our Galaxy were born in star clusters. These spherical groupings contain anywhere from a few tens to several million members all milling about under the influence of gravity. But their fate is sealed. All star clusters slowly dissolve over time. “The net effect of this is that their stars eventually become redistributed throughout the Galaxy,” said Nathan Leigh, a PhD student at McMaster University and lead author for a study being presented this week at the CASCA 2011 meeting in Ontario, Canada. “This is how we think most of the stars in the Milky Way came to be found in their currently observed locations.”
Although we now know that star clusters have played an important role in shaping the history of our Galaxy, we still do not understand how their stars are formed. Part of the problem lies in the fact that populations of young stars are typically hidden by a dense veil of gas and dust. This makes it very difficult to directly observe and study regions where stars are currently being born. In order to get around this, astronomers have combined observations of star clusters so old that they date back to the beginning of the Universe itself with state-of-the-art simulations for their evolution.
“Unfortunately, most star clusters take so long to dissolve that we cannot actually see it happening. But we now understand how this process occurs, and we can look for its signatures by examining the current appearances of clusters,” said Nathan Leigh. “We have gone about this by matching up the clusters we make with our simulations to the ones we actually observe. This tells us about the conditions at the time of their formation.”
This has allowed Leigh and collaborators to re-trace the histories of real star clusters, providing for the very first time a glimpse at their formation. To get the job done, they used highly sophisticated observations recently taken with the Hubble Space Telescope.
“Remarkably, we are finding that all star clusters more or less share a common history, extending all the way back to their births,” said Leigh. “This came as a big surprise to us since it suggests that the problem could be much simpler than we originally thought. Our understanding of not only how stars form, but also the history of our Galaxy, just took a much bigger step forward than we were expecting.”
# # #
Press Contacts:
Leslie Sage
CASCA Press Officer
+1 (301) 675-8957 (cell)
cascapressofficer@gmail.com
Michelle Donovan
Public Relations Manager
McMaster University
+1 (905) 525-9140 x22869
donovam@mcmaster.ca
Science Contacts:
Nathan Leigh
Department of Physics and Astronomy
McMaster University
+1 (905) 741-4557 (cell)
leighn@mcmaster.ca
Science Contacts (co-authors):
Alison Sills
Department of Physics and Astronomy
McMaster University
+1 (289) 244-5094 (cell)
asills@mcmaster.ca
Stefan Umbreit
NU Center for Interdisciplinary
Exploration and Research in Astrophysics
Northwestern University
+1 847-491-5626
s-umbreit@northwestern.edu
Christian Knigge
School of Physics & Astronomy
University of Southampton
+44 (0)23-8059-3955
c.knigge@soton.ac.uk
Links:
http://apod.nasa.gov/apod/ap021229.html
http://apod.nasa.gov/apod/ap020730.html
McMaster University, one of four Canadian universities listed among the Top 100 universities in the world, is renowned for its innovation in both learning and discovery. It has a student population of 23,000, and more than 140,000 alumni in 128 countries.
The University of Western Ontario is proudly hosting the 2011 CASCA conference May 30 to June 2, 2011, in London, Ontario, to celebrate Canadian astronomical and astrophysical research: http://www.casca2011.com/index.html
The Canadian Astronomical Society (http://www.casca.ca) was founded in 1971 and incorporated in 1983 as a society of professional astronomers. The society is devoted to the promotion and advancement of knowledge of the universe through research and education. Membership is open to persons with a professional involvement with these goals in astronomy and the related sciences. The main activities of the Society are its annual scientific meetings, the planning and realization of scientific projects, the support of the scientific activities of its members, and the dissemination of related information among members and other interested persons. The Society supports committees on Optical and Infrared Astronomy, Radio Astronomy, Space Astronomy, Theoretical Astronomy, Education, Heritage, Canadian Grad Students, and Awards. Cassiopeia, the quarterly newsletter of the Society, is published at equinoxes and solstices.
