'Galaxy interaction' presentation slideshows

Dynamics and star formation histories of the LMC and the SMC.

1.35k views • 118 slides

Rich cluster [M ~ 10 15 M sun ]

Environmental effects on neutral and molecular hydrogen of galaxies. (From APOD). Large groups (Small clusters) [M ~ 10 13 - 10 14 M sun ]. Small/compact groups [M < 10 13 M sun ]. Rich cluster [M ~ 10 15 M sun ]. Kenji Bekki (ICRAR at UWA, Australia).

478 views • 40 slides

Theoretical Aspects of Black hole-Galaxy Interaction

2014-02-10/12 SSG Workshop, ??. ??? ( ????? ??????? ). Theoretical Aspects of Black hole-Galaxy Interaction. I. Observational Facts. SMBHs exist in all galaxies, esp. with spheroids Kormendy & Richstone 1995 Richstone et al. 1998 Methods

289 views • 20 slides