"M dwarfs: planet formation and long term evolution" "M dwarfs: planet formation and long term evolution"
"Why the Smallest Stars Stay Small" "Why the Smallest Stars Stay Small"

من اشباه المفاعيل , هي

"The Fate of the Molecular Gas from Mergers to Ellipticals".

من اشباه المفاعيل , هي
"On the Evolution of Stars that Form Electron-degenerate Cores Processed by Carbon Burning
النجوم من أين تولد وكيف تموت؟ (مراحل حياة النجوم)
"On the Evolution of Stars that Form Electron-degenerate Cores Processed by Carbon Burning
من اشباه المفاعيل , هي
Paris, France: Kluwer Academic Publishers
Birth, Evolution and Death of Stars Tracing H 2 Via Infrared Dust Extinction
Paris, France: Kluwer Academic Publishers Birth, Evolution and Death of Stars

تطور النجوم

"On the Evolution of Stars that Form Electron-degenerate Cores Processed by Carbon Burning.

9
تطور النجوم
II — Characteristics of discrete features"
النجوم من أين تولد وكيف تموت؟ (مراحل حياة النجوم)
"The Structure and Evolution of Molecular Clouds: from Clumps to Cores to the IMF"
تطور النجوم