Planetary Sizes
Massive star feedback – from the first stars to the present
Asteroseismology of evolved stars: from hot B subdwarfs to white dwarfs
M Dwarfs as Targets for JWST
Atomic Spectroscopy for Space Applications: Galactic Evolution l M. P. Ruffoni, J. C. Pickering, G. Nave, C. Allende-Prieto.
Www.upc.edu The white dwarf cooling age of NGC 6791 Enrique García-Berro, Santiago Torres, Leandro Althaus, Isabel Renedo, Pablo Lorén-Aguilar, Alejandro.
Gianluca Imbriani Physics Department of University of Naples Federico II, Italian National Institute of Nuclear Physics (INFN) and Joint Institute of Nuclear.
The Secondary Stars of Cataclysmic Variables
PRESUPERNOVA EVOLUTION AND EXPLOSION OF MASSIVE STARS: CHALLENGES OF THE NEXT CENTURY
1/34 PRESUPERNOVA EVOLUTION AND EXPLOSION OF MASSIVE STARS: CHALLENGES OF THE NEXT CENTURY Marco Limongi INAF – Osservatorio Astronomico di Roma, ITALY.
The Sun A Model Star. Factoids to Start: Official name: Sol (as in Solar System) 1.5 X 10 11 meters distant (93 million miles, 8.3 light minutes) Size:
Insights in stars, neutrino physics and in the Earth
