Slide 1 Deep Convective Clouds and Chemistry (DC3)* Field campaign to study the impact of midlatitude deep convection on the upper troposphere-lower stratosphere (UT-LS)…

Slide 1 The birth of a star Chapter 11 1.Where are the birth places of stars? 2.What are the main components of a protostar? 3.When and how a new is born? 4.What prevents…

Slide 1 1 As hydrogen is exhausted in the (convective) core of a star (point 2) it moves away from the main sequence (point 3) What happens to the star ? lower T  redder…

Slide 1 1) Deeper comparison of the case 1.4 Parameters: M/M O =2.0 X 0 =0.70 Y 0 =0.28 Z 0 =0.02 l MLT /H p =1.6 Target model: T c =1.9. 10 7 K (PMS) Tests and future plans…

Slide 1 Improving our understanding of Stellar Evolution with PLATO 2.0 Santi Cassisi INAF - Astronomical Observatory of Teramo, Italy Slide 2 PLATO2.0 Stellar Evolution…

Slide 1 Origin of the elements and Standard Abundance Distribution Clementina Sasso Lotfi Yelles Chaouche Lecture on the Origins of the Solar Systems Slide 2 Nucleosynthesis:…

The birth of a star Chapter 11 Where are the birth places of stars? What are the main components of a protostar? When and how a new is born? What prevents a star from collapsing?…

Slide 1 New Insights on the origin of Magnetic Fields in White Dwarfs Dayal Wickramasinghe and Lilia Ferrario Australian National University Canberra The chemically peculiar…

1) Deeper comparison of the case 1.4 Parameters: M/MO=2.0 X0=0.70 Y0=0.28 Z0=0.02 lMLT/Hp=1.6 Target model: Tc=1.9.107 K (PMS) Tests and future plans for the FRANEC code…

Bit of Administration â¦. Reading BSNV Chap. 12 Homework 9 Due Friday, April 23, in box by Mathieu office door (6522) Sterling Portfolios Due Wednesday, April 28 Can turn…