Slide 1Millimeter-Wavelength Observations of Circumstellar Disks and what they can tell us about planets A. Meredith Hughes Miller Fellow, UC Berkeley David Wilner, Sean…

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Slide 1Core Collapse SNe Inma Domínguez Marco Limongi Slide 2  Evolution of Massive Stars  Hydrostatic Nucleosynthesis  Explosion Mechanism  Explosive Nucleosynthesis…

Slide 1Chapter 12. Star Stuff (mostly different from book) I. Birth of Stars from Interstellar Clouds Young stars near clouds of gas and dust Contraction and heating of clouds…

Slide 1 Studying circumstellar envelopes with ALMA David Neufeld Johns Hopkins University Slide 2 The 0.1 – 10 4  m background Since t = 10 5 yr, most of the photons…

Slide 1 Post-AGB evolution Slide 2 Learning outcome evolution from the tip of the AGB to the WD stage object types along the post-AGB evolution basics about planetary nebulae…

Slide 1 Stellar Astrophysics with the Keck Interferometer PI: S. R. Kulkarni Co-I’s: D. Sasselov, M. Konacki, B. Lane Slide 2 Motivation Current stellar models –Current…

Pulsation models: Cepheids and RR Lyrae Marcella Marconi INAF Astronomical Observatory of Capodimonte,Naples,Italy S. Agata sui due Golfi, May 2005 Outline S. Agata sui due…

Formation and Early Evolution of Intermediate-Mass Stars Intermediate-Mass Stars in the Context Clustering and the Formation of “Early”-Type Systems Disks as a probe…

Studying circumstellar envelopes with ALMA David Neufeld Johns Hopkins University The 0.1 – 104 mm background Since t = 105 yr, most of the photons generated in the Universe…