Documents Rich cluster [M ~ 10 15 M sun ] Large groups (Small clusters) [M ~ 10 13 - 10 14 M sun ]...

Slide 1 Rich cluster [M ~ 10 15 M sun ] Large groups (Small clusters) [M ~ 10 13 - 10 14 M sun ] Environmental effects on neutral and molecular hydrogen of galaxies Small/compact…

Documents Helioseismic Magnetic Imager and Why We Study Helioseismology Junwei Zhao W. W. Hansen Experimental....

Slide 1 Helioseismic Magnetic Imager and Why We Study Helioseismology Junwei Zhao W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA94305-4085…