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M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture07.pdf23 Oct 2023: Tb. Ho. Er. Tm. Yb. Hf. Dy. Figure 1.— Recent abundance determinations in five r-process rich stars, based upon new atomiclab data, compared with two solar system r-process only -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture16.pdf24 Nov 2023: 16.1 A Little History. In 1572 the Danish astronomer Tycho Brahe observed a new star in theconstellation of Cassiopeia and described it in his book De Stella Nova(Latin for ... Concerning the New Star”), giving rise to the name nova.Novae are now -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture11.pdf6 Nov 2023: Thus a new star is chemically homogeneous. This will change asthe star ages.
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