Focusing in on the Galactic Center – Dr. Mark Morris

(January 25, 2011)  Three of the most massive star clusters in our Milky Way Galaxy are found near the Galaxy’s center and their formation dynamics produce a startling display of pyrotechnics.  Alongside these young compact star groups, the Galactic Center also harbors the Milky Way’s massive black hole putting forth many fascinating mysteries; for one, how can stars form so close to the hostile environment of a supermassive black hole.  UCLA Professor Mark Morris will present current research findings from observations made with the Keck telescopes and their adaptive optics systems to resolve these complex questions of the cosmos.

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UCLA observers will work with MOSFIRE tonight. And UCI/UCB observers will work with NIRC2-LGS/NIRC2-NGS. Sun set 05:59:00pm rise 06:12:00am
Observers from UCR will use MOSFIRE on Keck 1, while on Keck 2, UCI observers will use DEIMOS. Sun set 06:00:00pm rise 06:12:00am
On Keck 1, we have UCR observers using LRIS-ADC. On Keck 2, we have Swinburne observers using ESI. Sun set 06:00:00pm rise 06:11:00am
CIT observers will use LRISP-ADC on Keck 1, and UCSC observers will use ESI on Keck 2 tonight. Sun set 06:01:00pm rise 06:11:00am
Our guests tonight are observers from UCSC and Swinburne, using LRISP-ADC and DEIMOS respectively. Sun set 06:02:00pm rise 06:10:00am