Current Challenges in Multi-Scale AnalysisJanuary 15 and 16, 2003 |
![]() Chandra's image of the elliptical galaxy NGC 4697 reveals diffuse hot gas dotted with many point-like sources. As in the elliptical galaxies, NGC 4649 and NGC 1553, the point-like sources are due to black holes and neutron stars in binary star systems. |
The workshop will follow-up on a Special Session at the American Astronomical Society Meeting in Seattle (January 2003) and aims to:
All with the goal of reporting back to the wider astronomical community. |
Scientific Organizing ComitteeAlanna Connors, Eureka ScientificPeter Freeman, CXC/CfAMargarita Karovska, CXC/CfAVinay Kashyap, CXC/CfAEric Kolaczyk, Boston UniversityAneta Siemiginowska, CXC/CfADavid van Dyk, Harvard University |
Astronomers
Albert Bijaoui
| StatisticiansEric KolaczykDavid Esch
| Engineering and Nuclear MedicineBecca WillettClem Karl |
![]() The Crab Nebula X-ray Chandra |
![]() The Crab Nebula Optical Palomar |
![]() G21.5-0.9 X-ray Chandra |
![]() E0102-72.3 X-ray Chandra |