- Bipolar Flows from Young Stars
Many, perhaps all, young stars generate bipolar outflows as they accrete mass. Bipolar outflows can be enormous structures, but the engines driving them are quite compact.
http://www.drao.nrc.ca/science/ska/futures_report/node67.html
(Added: Sat Oct 26 2002)
- Chandrasekhar Limit
Around 1930, S. Chandrasekhar studied astrophysical models of white dwarf stars and came to the conclusion that no white dwarf can be more massive than about 1.4 solar masses.
http://scienceworld.wolfram.com/physics/ChandrasekharLimit.html
(Added: Sat Oct 26 2002)
- Protostar Article
“Stellar embryology” takes a step forward with the first detailed look at the youngest Sun-like stars. This is an article by Thomas Greene.
http://www.sigmaxi.org/amsci/articles/01articles/Greene.html
(Added: Sat Oct 26 2002)
- Protostars
T Tauri stars are young, solar-like stars seen near many molecular clouds in our galaxy.
http://etacha.as.arizona.edu/~eem/ttau/yso.html
(Added: Sat Oct 26 2002)
- T Tauri
A T Tauri star is a very young (pre-main sequence) star thought to only recently have emerged from the cocoon of gas in which it formed.
http://zebu.uoregon.edu/~imamura/208/feb15/tauri.html
(Added: Sat Oct 26 2002)
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