Time |
Speaker |
Affiliation |
Title |
Presentation |
7:45a | | |
Bus leaves from the Courtyard North to the Omni. |
  |
8:00-9:00a | | |
Continental Breakfast, Poster Set-up,
pick-up workshop registration materials. |
  |
9:00-9:15a | Fred Lo | NRAO - CV |
Welcome and Scientific Overview |
PDF |
9:15-9:45a | Paolo Padoan | University of California, San Diego |
The formation of molecular cores from turbulent flows |
PDF;
movie
|
9:45-10:15a | Neal Evans | University of Texas |
Observed properties of massive molecular cores |
PDF |
10:15-10:35a | Frederique Motte | AIM/SAp, CEA Saclay |
Properties of high-mass protostars and massive pre-stellar cores at
the dawn of Herschel and ALMA |
PDF |
10:35-11:05a | | |
Coffee Break |
|
11:05-11:35a | Jonathan Tan | University of Florida |
The formation of high mass stars from cores |
PDF |
11:35-12:05p | Crystal Brogan | NRAO |
Observational constraints on massive star formation |
PDF |
12:05-12:25p | Qizhou Zhang | CfA |
Fragmentation in (Pre)cluster Forming Regions |
PDF |
12:25-12:35p | | |
Discussion |
|
12:35-2:05p | | |
Lunch |
|
2:05-2:25p | Philippe Andre | CEA/SAp Saclay |
Probing the earliest stages of massive star formation in cluster-forming clumps |
PDF |
2:25-2:55p | Daniela Calzetti | University of Massachusetts |
Scaling relations for star formation and feedback on galaxy scales |
PDF |
2:55-3:15p | Adam Leroy | MPIA |
The star formation efficiency in nearby galaxies: results from THINGS++ |
PDF |
3:15-3:45p | | |
Coffee Break |
|
3:45-4:05p | Konstantinos Tassis | KICP |
Using cosmological simulations to connect star formation in molecular clouds with observations on galactic scales |
PDF |
4:05-4:25p | Yancy Shirley | University of Arizona |
Constant SFR/M in high-mass star-forming clumps |
PDF |
4:25-4:45p | Desika Narayanan | Harvard-Smithsonian Center for Astrophysics |
Molecular star formation rate indicators in galaxies |
PDF;
movie1;
movie2;
movie3
|
4:45-5:05p | Guinevere Kauffmann | Max Planck Institute for Astrophysics |
Evidence that the top end of the IMF varies in nearby star-forming galaxies |
PDF |
5:05-5:15p | | |
Discussion |
|
5:30 & 5:45p | | |
Buses leave from
the Omni to the NTC. |
|
6:00-8:00p | | |
Director's reception/tour of NRAO Technology Center.
|
|
8:00p | | |
Buses leave from the NTC to
the Omni and Marriot Courtyard North. |
|
|
Friday, September 26: |
Time |
Speaker |
Affiliation |
Title |
Presentation |
8:00a | | |
Bus leaves from the Courtyard North to the Omni. |
  |
8:00-9:00a | | |
Continental Breakfast |
  |
9:00-9:20a | Floris van der Tak | SRON |
Chemical evolution of massive star-forming regions |
PDF |
9:20-9:40a | Peter Schilke | MPIfR |
What are the best (molecular) tracers of physical conditions in
regions of massive star formation? |
N/A |
9:40-10:00a | Ramprasad Rao | Submillimeter Array/ASIAA |
Submillimeter Array observations of magnetic fields in massive star
forming regions |
N/A |
10:00-10:20a | Zhi-Yun Li | University of Virginia |
Outflow feedback in cluster formation |
PDF;
movie
|
10:20-11:00a | | |
Coffee Break |
  |
11:00-11:20a | Keping Qiu | Harvard-Smithsonian Center for Astrophysics |
Submillimeter Array observations of molecular outflows in massive star
forming regions |
PDF |
11:20-11:40a | Christopher Matzner | University of Toronto |
When and how does protostellar dynamical feedback matter? |
PDF |
11:40a-12:00p | Eric Keto | Harvard-Smithsonian Center for Astrophysics |
The Formation of Massive Star Clusters by Cooperative Accretion |
PDF |
12:00-12:20p | Mark Krumholz | UC Santa Cruz |
What does it take to make a massive star? |
PDF;
movie1;
movie2;
movie3
|
12:20-12:30p | | |
Discussion |
  |
12:30-2:00p | | |
Lunch |
  |
2:00-2:20p | John Bally | University of Colorado, Boulder |
Feedback from massive stars |
PDF |
2:20-2:40p | Ed Churchwell | University of Wisconsin-Madison |
Dusty, wind-blown bubbles: Not your classical HII region |
PDF |
2:40-3:00p | Annie Zavagno | LAM |
Star formation triggered by Galactic HII regions |
N/A |
3:00-3:20p | Leisa Townsley | Penn State University |
X-ray observations of massive star formation and feedback |
PDF |
3:20-4:00p | | |
Coffee Break |
  |
4:00-4:20p | Mark Westmoquette | University College London |
Spatially-resolved studies of super star cluster feedback in starburst galaxies |
N/A |
4:20-4:50p | Tim Heckman | Johns Hopkins |
What drives galaxy-scale feedback? |
PDF |
4:50-5:10p | Eva Schinnerer | MPIA |
Tracing nuclear star formation and feedback |
PDF |
5:10-5:30p | Daniel Weisz | University of Minnesota |
Triggered star formation in M81 group dwarf galaxy IC2574 |
PDF;
movie |
5:30-5:40p | | |
Discussion |
  |
5:40-7:00p | | |
Poster
Viewing Session with wine and cheese - Omni Hotel, Room 225. |
  |
7:00-9:00p | | |
Conference
Dinner-Omni Hotel Atrium; Sponsored by UVa Astronomy
Department. |
  |
9:15 & 10:00p | | |
Buses leave
from the Omni to the Courtyard North. |
  |
|
Saturday, September 27: |
Time |
Speaker |
Affiliation |
Title |
Presentation |
8:00a | | |
Bus leaves from the Courtyard North to the Omni. |
  |
8:00-9:00a | | |
Continental Breakfast |
  |
9:00-9:20a | Alison Peck | ALMA |
Current status of ALMA |
PDF |
9:20-9:40a | Maria Cunningham | University of New South Wales |
Turbulence, feedback, and star formation in the G333 molecular cloud complex |
PDF |
9:40-10:00a | Nathan Smith | UC Berkeley |
A potential bonanza for ALMA in the Carina Nebula |
PDF |
10:00-10:20a | Farhad Yusef-Zadeh | Northwestern University |
Star formation in the Galactic Center region |
PDF |
10:20-10:50a | | |
Coffee Break |
  |
10:50-11:10a | Yasuo Fukui | Nagoya University |
What are the conditions for forming massive star clusters:
lessons in the GC and the LMC |
PDF |
11:10-11:30a | Alberto Bolatto | University of Maryland |
The properties of extragalactic GMCs |
PDF |
11:30-11:50a | Chris Wilson | McMaster University |
Massive star formation in extreme environments |
PDF |
11:50a-12:00p | | |
Discussion |
  |
12:00-1:30p | | |
Lunch |
  |
1:30-2:00p | Adrian Russell | ALMA/NRAO-CV |
The future evolution of ALMA |
PDF |
2:00-3:30p | | |
Discussion (Thematic groups
on development science drivers) |
  |
3:30-4:30p | | |
Discussion (all) |
  |
4:30p | | |
Bus leave
from the Omni to the Courtyard North. |
  |