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M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture03.pdf10 Oct 2023: levels.Eventually the electron will de-excite and jump down to a lower energylevel, emitting a new photon of specific frequency. -
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 -
MNRAS 000, 1–11 (2023) Preprint 31March 2023 Compiled…
https://people.ast.cam.ac.uk/~wyatt/mmcb23.pdf31 Mar 2023: 2014;Hagan et al. 2018), which allowed the discov-ery of 12 other new debris discs in scattered light (Soummer et al.2014; Choquet et al. ... Figure 3. Spectral energy distribution of HD 16743. White data points areancillary photometry from the literature -
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. -
MNRAS 000, 1–16 (2022) Preprint 6 July 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf11 Jul 2023: 2018, e.g. cometC/2016 R2)). The recent New Horizons fly-by of Arrokothplaced upper limits on the release of hyper-volatiles (CO,. ... Jutzi & Benz 2017; Davidsson 2023).Collisions also expose new surface, such that volatiles canbe lost via sublimation -
The clumpy structure of epsilon Eridani's debris disc revisited…
https://people.ast.cam.ac.uk/~wyatt/bpkw23.pdf27 Mar 2023: the disc features.In this paper we present new ALMA observations of the. ... This allowed us to consider dif-ferent initial disc setups by varying the disc parameters in apost-processing step, without having to run a new simulationfor each setup.
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