International Virtual Observatory Alliance

Difference: TheoryIntScale (1 vs. 2)

Revision 22012-06-26 - root

META TOPICPARENT	name="IvoaTheoryUseCases"

Intermediate Scale Theory Use Cases

Description of two examples of intermediate scale numerical simulations of very different astrophysical problems. The first problem addresses the evolution of globular clusters, where the dynamical and stellar evolution is followed for every star in the cluster. The second problem describes the evolution of extragalactic jets, both energetic FRII MHD jets and less energetic FRI MHD jets in clusters of galaxies that form buoyant bubbles in the intracluster medium.

META FILEATTACHMENT	attr="" comment="IVOA oct 2005 presentation" date="1128590807" name="IVOATheory0905.ppt" path="IVOATheory0905.ppt" size="929792" user="PeterTeuben" version="1.1"
META FILEATTACHMENT	attr="" comment="Magnetic field" date="1128590866" name="HB5ka.mpeg" path="HB5ka.mpeg" size="1883612" user="PeterTeuben" version="1.1"
META FILEATTACHMENT	attr="" comment="Tracer of radio source material" date="1128590946" name="HB5kc.mpeg" path="HB5kc.mpeg" size="1534589" user="PeterTeuben" version="1.1"

Revision 12005-10-06 - PeterTeuben

META TOPICPARENT	name="IvoaTheoryUseCases"

Intermediate Scale Theory Use Cases

<-- 
 
 
 Set ALLOWTOPICRENAME = TWikiAdminGroup
 
 
-->

META FILEATTACHMENT	attr="" comment="IVOA oct 2005 presentation" date="1128590807" name="IVOATheory0905.ppt" path="IVOATheory0905.ppt" size="929792" user="PeterTeuben" version="1.1"
META FILEATTACHMENT	attr="" comment="Magnetic field" date="1128590866" name="HB5ka.mpeg" path="HB5ka.mpeg" size="1883612" user="PeterTeuben" version="1.1"
META FILEATTACHMENT	attr="" comment="Tracer of radio source material" date="1128590946" name="HB5kc.mpeg" path="HB5kc.mpeg" size="1534589" user="PeterTeuben" version="1.1"

View topic | History: r2 < r1 | More topic actions...