New pre-main-sequence tracks for M less than or equal to 2.5 solar mass as tests of opacities and convecti on model
@article{Dantona1994NewPT, title={New pre-main-sequence tracks for M less than or equal to 2.5 solar mass as tests of opacities and convecti on model}, author={F. D'antona and I. Mazzitelli}, journal={Astrophysical Journal Supplement Series}, year={1994}, volume={90}, pages={467-500} }
578 Citations
Testing the Chronometric Accuracy of Stellar Evolution Models Using Young Stars in Open Clusters
- Physics
- 2010
- 1
- Highly Influenced
- PDF
Influence of Dust Grain Evolution on the Structure of Protoplanetary Disks.
- Geology
- 2014
- Highly Influenced
MASS ESTIMATES FOR GALACTIC DARK MATTER OBJECTS AS A TEST OF A FRACTAL COSMOLOGICAL PARADIGM
- Physics
- 2002
- 4
- Highly Influenced
- PDF
Keck Diffraction-limited Imaging of the Young Quadruple Star System HD 98800
- Physics
- 2001
- 46
- Highly Influenced
- PDF
Dynamical Masses of T Tauri Stars and Calibration of Pre-Main-Sequence Evolution
- Physics
- 2000
- 346
- Highly Influenced
- PDF