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Monash chemical yie...
Monash chemical yields project (Monχey) element production in low- and intermediate-mass stars
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- Doherty, Carolyn L. (författare)
- Monash University
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- Lattanzio, John (författare)
- Monash University
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- Angelou, George (författare)
- Max Planck Institute for Solar System Research
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- Campbell, Simon W. (författare)
- Monash University
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- Church, Ross (författare)
- Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
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- Constantino, Thomas N. (författare)
- Monash University
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- Cristallo, Sergio (författare)
- INAF Osservatorio Astronomico di Teramo
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- Gil-Pons, Pilar (författare)
- Polytechnic University of Catalonia
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- Karakas, Amanda (författare)
- Australian National University
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- Lugaro, Maria (författare)
- Research Centre For Astronomy and Earth Sciences, Hungarian Academy of Sciences
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- Stancliffe, Richard J. (författare)
- University of Bonn
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(creator_code:org_t)
- 2015
- 2015
- Engelska 2 s.
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Ingår i: Proceedings of the International Astronomical Union. - 1743-9213. ; 11:A29B, s. 164-165
- Relaterad länk:
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http://dx.doi.org/10...
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https://lup.lub.lu.s...
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https://doi.org/10.1...
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Abstract
Ämnesord
Stäng
- The Monχey project will provide a large and homogeneous set of stellar yields for the low- and intermediate- mass stars and has applications particularly to galactic chemical evolution modelling. We describe our detailed grid of stellar evolutionary models and corresponding nucleosynthetic yields for stars of initial mass 0.8 M⊙ up to the limit for core collapse supernova (CC-SN) ≈ 10 M⊙. Our study covers a broad range of metallicities, ranging from the first, primordial stars (Z = 0) to those of super-solar metallicity (Z = 0.04). The models are evolved from the zero-age main-sequence until the end of the asymptotic giant branch (AGB) and the nucleosynthesis calculations include all elements from H to Bi. A major innovation of our work is the first complete grid of heavy element nucleosynthetic predictions for primordial AGB stars as well as the inclusion of extra-mixing processes (in this case thermohaline) during the red giant branch. We provide a broad overview of our results with implications for galactic chemical evolution as well as highlight interesting results such as heavy element production in dredge-out events of super-AGB stars. We briefly introduce our forthcoming web-based database which provides the evolutionary tracks, structural properties, internal/surface nucleosynthetic compositions and stellar yields. Our web interface includes user- driven plotting capabilities with output available in a range of formats. Our nucleosynthetic results will be available for further use in post processing calculations for dust production yields.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Nyckelord
- abundances
- nuclear reactions
- nucleosynthesis
- stars: AGB and post-AGB
Publikations- och innehållstyp
- art (ämneskategori)
- ref (ämneskategori)
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Till lärosätets databas
- Av författaren/redakt...
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Doherty, Carolyn ...
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Lattanzio, John
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Angelou, George
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Campbell, Simon ...
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Church, Ross
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Constantino, Tho ...
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visa fler...
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Cristallo, Sergi ...
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Gil-Pons, Pilar
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Karakas, Amanda
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Lugaro, Maria
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Stancliffe, Rich ...
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visa färre...
- Om ämnet
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- NATURVETENSKAP
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NATURVETENSKAP
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Lunds universitet