Slide 1Physical conditions of the shocked regions in collimated outflows of planetary nebulae Angels Riera (UPC) Slide 2 OUTLINE Identification: morphology and kinematics.…

Slide 1 1 Black Hole Masses from Reverberation Mapping Bradley M. Peterson The Ohio State University Collaborators: M. Bentz, S. Collin, K. Dasyra, K. Denney, L. Ferrarese,…

Massive star feedback – from the first stars to the present Jorick Vink (Keele University) Outline Why predict Mass-loss rates? (as a function of Z) Monte Carlo Method…

Massive star feedback – from the first stars to the present Jorick Vink (Keele University) Outline Why predict Mass-loss rates? (as a function of Z) Monte Carlo Method…

Black Hole Masses from Reverberation Mapping Bradley M. Peterson The Ohio State University Collaborators: M. Bentz, S. Collin, K. Dasyra, K. Denney, L. Ferrarese, K. Horne,…

Physical conditions of the shocked regions in collimated outflows of planetary nebulae Angels Riera (UPC) OUTLINE Identification: morphology and kinematics. Physical conditions…

Slide 1 + Criteria for Candidates Altitude > 40°; Apparent Magnitude > 14; Available Distance and Angular Radius; Available Spectra Introduction Planetary nebulae…