The Stellar Birthline

ePAPER READ

DOWNLOAD ePAPER

astro1.physics.utoledo.edu

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

START NOW

The Effect of Surface Cooling

Hartmann et al 1997

Sunday, May 1, 2011

Lecture 6: Modeling Molecular Cores as Bonnor-Ebert Spheres and ...

Lecture 25: Pulsating Stars, Cepheids and RR-Lyrae Stars

calculation of mean atomic weight of an ionized gas

Lecture 3 Properties and Evolution of Molecular Clouds

Lecture 4 Turbulence and Magnetic Fields in Molecular Clouds

Lecture 9: The Spectral Energy Distributions of Dusty Young Stellar ...

Lecture 24: AGB Stars and Massive Star Evolution

Lecture 29: The End Stages of Massive Stars and Supernovae

Stellar birthline for total luminosity L=0 This shows the evolution of central temperature and f, the fraction of D/H (relative to the interstellar abundance.) core temperature Hartmann et al 1997 fraction of Deuterium Sunday, May 1, 2011

The Effect of Surface Cooling Hartmann et al 1997 Sunday, May 1, 2011

Page 1 and 2: Lecture 19: Protostars & the Stella
Page 3 and 4: Decreasing Luminosity Increasing Ti
Page 5 and 6: Review: Convective Pre-Main Sequenc
Page 7 and 8: Convective (Hayashi) Track Radiativ
Page 9 and 10: Now go to protostellar phase 9 Sund
Page 11 and 12: The Stellar Birthline 11 Sunday, Ma
Page 13 and 14: We define α: 13 Sunday, May 1, 201
Page 15 and 16: Sunday, May 1, 2011 15
Page 17: Hartmann et al 1997 Stellar Birthli
Page 21: Summary The Stellar Birthline is th

The Stellar Birthline

Create successful ePaper yourself

Delete template?

Save as template?