The Globular Cluster-Galaxy Connection 1 st meeting: July 1992; Globular Clusters Within the Context of Their Parent Galaxies 2 nd meeting: July 2011;
Chapter 15 – Measuring Pressure (con’t) Temperature spans a factor of 10 or so from M to O stars Pressure/luminosity spans six orders of magnitude from.
Modelling the Milky Way James Binney Oxford University TexPoint fonts used in EMF. Read the TexPoint manual before you delete this box.: AAA A A A A A.
The UV properties of elliptical galaxies A. Gil de Paz (UCM), B.F. Madore (OCIW), S. Boissier, A. Boselli, J. Donas, J.M. Deharveng (LAM), R. Michael Rich.
Chapter 15 – Measuring Pressure (con’t)
The Milky Way Galaxy James Binney Oxford University.
AGB stars in Galactic Globular Clusters – Are They Chemically Distinct to Their Fellow RGB and HB Stars?
Pulsation models: Cepheids and RR Lyrae Marcella Marconi INAF Astronomical Observatory of Capodimonte,Naples,Italy S. Agata sui due Golfi, May 2005.
The Globular Cluster-Galaxy Connection
