Xavier Barcons Instituto de Física de Cantabria (CSIC-UC) On behalf of The Athena+ Co-ordination Group, the Athena+ Working Groups and Supporters A theme.
PROBING THE MILKY WAYS OXYGEN GRADIENT WITH PLANETARY NEBULAE Dick Henry H.L. Dodge Department of Physics & Astronomy University of Oklahoma Collaborators:
The Formation of Stars Chapter 11. Previous chapters have used the basic principles of physics as a way to deduce things about stars and the interstellar.
The International Heliophysical Year and Universal Processes In Space Science Acknowledgments: Crooker, Davila, Fuller-Rowell, Gopalswamy, Onsager, Siscoe,
Chapter 5: Cosmic foundations for origins of life - stars.
What can emission lines tell us? lecture 1 Grażyna Stasińska.
Star Formation Why is the sunset red? The stuff between the stars Nebulae Giant molecular clouds Gravitational collapse of molecular cloud Gravitational.
29 March 2005AST 2010: Chapter 191 Between the Stars: Gas & Dust in Space.
An introduction to the physics of the interstellar medium I. Overview II. Thermal processes in the ISM III. Hydrodynamics in the ISM IV. Gravity in the.
The Formation and Structure of Stars Chapter 9. The Big Picture Stars exist because of gravity. Gravity causes interstellar material to collapse to form.
Stellar Winds and their Interaction with the Interstellar Medium Brian E. Wood (Naval Research Laboratory) Jeffrey L. Linsky (JILA, University of Colorado)
Timing Analysis of the Isolated Neutron Star RXJ0720.4–3125 Silvia Zane, Frank Haberl, Mark Cropper, Vyacheslav Zavlin, David Lumb, Steve Sembay & Christian.
