The Stellar Birthline

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Hartmann et al 1997

Stellar Birthline for total luminosity L=0 and two different

accretion rates.

Different values of α are used in the left panel.

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

Now we can write: 16 Sunday, May 1, 2011

Hartmann et al 1997 Stellar Birthline for total luminosity L=0 and two different accretion rates. Different values of α are used in the left panel. 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: Sunday, May 1, 2011 15
Page 19 and 20: The Effect of Surface Cooling Hartm
Page 21: Summary The Stellar Birthline is th

The Stellar Birthline

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