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  3. ASTRONOMY COLLOQUIUM<br>Star Clusters and High Mass X-Ray Binaries in Nearby Spirals, Mergers, and Starburst Galaxies
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ASTRONOMY COLLOQUIUM<br>Star Clusters and High Mass X-Ray Binaries in Nearby Spirals, Mergers, and Starburst Galaxies

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        3. <b>ASTRONOMY COLLOQUIUM</b><br>Tracing the Cosmic Shutdown of Star Formation in Massive Galaxies
        4. <b>ASTRONOMY COLLOQUIUM</b><br>The Effects of Magnetic Field Morphology on the Determination of Oxygen and Iron Abundances in the Solar Photosphere
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        6. <b>ASTRONOMY COLLOQUIUM</b><br>Lonely Galaxies: The Baryon Content of Isolated Dwarf Galaxies
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        17. ASTRONOMY COLLOQUIUM<br>Blowing in the Quasar Wind: Feedback from Black Hole Outflows in Major Galaxy Mergers
        18. ASTRONOMY COLLOQUIUM<br>Magellan/MDM Colloquium: Department Members Share Their Current Work Using Magellan/MDM Observatories
        19. ASTRONOMY COLLOQUIUM<br>The Fisk-Vanderbilt Masters-to-PhD Bridge Program: A Model for Increasing Diversity at the PhD Level in Physics & Astronomy
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        21. ASTRONOMY COLLOQUIUM<br>Observing the Formation of Planetary Diversity
        22. ASTRONOMY COLLOQUIUM<br>Lies, Damned Lies, and Statistics: Empirical Constraints on Theories of Planet Formation
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        24. ASTRONOMY COLLOQUIUM <br> Hot on the Trail of Warm Planets Orbiting Cool Stars
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        45. ASTRONOMY COLLOQUIUM<br>3D Spectroscopy of Giant H II Regions in Nearby Spiral Galaxies</br>
        46. ASTRONOMY COLLOQUIUM<br>Star Clusters and High Mass X-Ray Binaries in Nearby Spirals, Mergers, and Starburst Galaxies
        47. PUBLIC ASTRONOMY DISTINGUISHED ALUMNUS COLLOQUIUM | Cracking the Cosmic Code
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Thursday, January 23, 2014
5:00 AM
807 Dennison Building

There is now strong evidence that many and possibly most stars form in clusters, rather than individually. This means that most of the massive stars that we observe in galaxies have, at some point, lived in a star cluster, and that the life cycle of star clusters tells us about the build up of galaxies. Motivated by observations of nearby spirals, mergers, and starburst galaxies taken with the Hubble Space Telescope, I will discuss recent results which address the following issues: 

(1) The mass and age distributions of star clusters tell us about the formation and disruption of the clusters. Are these distributions similar in different galaxies? 

(2) High mass x-ray binaries (HMXBs), where either a black hole or neutron star is closely orbited by a massive star, trace recent star formation in galaxies, and are often found close to star clusters. What is the relationship between HMXBs and star clusters? 

(3) The inter-arm regions of spiral galaxies emit diffuse, ultraviolet light. Are low-mass star clusters responsible for this emission?

Astronomy Colloquia listings for Winter 2014.

Speaker:
Physics
Randall Lab and Homer A. Neal Lab
450 Church Street
Ann Arbor, MI 48109-1040
734.764.4437
734.763.9694
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