Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Melanie Hampel"'
Autor:
Arthur Choplin, A. Skuladottir, Camilla Juul Hansen, Stefania Salvadori, Simon Campbell, Melanie Hampel
The slow ($s$) and intermediate ($i$) neutron ($n$) capture processes occur both in asymptotic giant branch (AGB) stars, and in massive stars. To study the build-up of the $s$- and $i$-products at low metallicity, we investigate the abundances of Y,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::deaa85c882c1370034b4375db126a078
http://arxiv.org/abs/1912.06671
http://arxiv.org/abs/1912.06671
Publikováno v:
Springer Proceedings in Physics ISBN: 9783030138752
We examine the observed heavy-element abundances of two types of objects that show enrichments in s-process elements but whose abundance patterns are generally incompatible with s-process predictions: CEMP-i stars and Pb-poor post-AGB stars, with rep
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c899a74eb87dae524eb991bbbf9238f9
https://doi.org/10.1007/978-3-030-13876-9_66
https://doi.org/10.1007/978-3-030-13876-9_66
Autor:
Richard J. Stancliffe, Melanie Hampel, Andreas Koch, Almudena Arcones, Camilla Juul Hansen, Moritz Reichert, Amanda I. Karakas
Publikováno v:
Astronomy and Astrophysics
Koch, A, Reichert, M, Hansen, C J, Hampel, M, Stancliffe, R J, Karakas, A & Arcones, A 2019, ' Unusual neutron-capture nucleosynthesis in a carbon-rich Galactic bulge star ', Astronomy & Astrophysics, vol. 622, A159 . https://doi.org/10.1051/0004-6361/201834241
Astronomy and astrophysics 622, A159-(2019). doi:10.1051/0004-6361/201834241
Astronomy & Astrophysics
Koch, A, Reichert, M, Hansen, C J, Hampel, M, Stancliffe, R J, Karakas, A & Arcones, A 2019, ' Unusual neutron-capture nucleosynthesis in a carbon-rich Galactic bulge star ', Astronomy & Astrophysics, vol. 622, A159 . https://doi.org/10.1051/0004-6361/201834241
Astronomy and astrophysics 622, A159-(2019). doi:10.1051/0004-6361/201834241
Astronomy & Astrophysics
Metal-poor stars in the Galactic halo often show strong enhancements in carbon and/or neutron-capture elements. However, the Galactic bulge is notable for its paucity of carbon-enhanced metal-poor (CEMP) and/or CH-stars, with only two such objects kn
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a00a83c84cc2ca992901dc4087db3b8f
Publikováno v:
Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016).
Publikováno v:
The Astrophysical Journal. 887:11
Lead (Pb) is predominantly produced by the slow neutron-capture process (s process) in asymptotic giant branch (AGB) stars. In contrast to significantly enhanced Pb abundances predicted by low-mass, low-metallicity AGB-models, observations of Magella
Carbon-enhanced metal-poor (CEMP) stars in the Galactic Halo display enrichments in heavy elements associated with either the s (slow) or the r (rapid) neutron-capture process (e.g., barium and europium respectively), and in some cases they display e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f62fadd62a6bf2d881fa607e6edd090
We present a new theoretical estimate for the birthrate of R Coronae Borealis (RCB) stars that is in agreement with recent observational data. We find the current Galactic birthrate of RCB stars to be $\approx$ 25% of the Galactic rate of Type Ia sup
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::86bb0bf36541489767d1aadf73b8732d
http://arxiv.org/abs/1507.06367
http://arxiv.org/abs/1507.06367
Publikováno v:
Astrophysical Journal; 12/10/2019, Vol. 887 Issue 1, p1-1, 1p
Autor:
Blanka Világos, Melanie Hampel, G. Tagliente, Valentina D'Orazi, F. Dell'Agli, U. Battino, Paolo Ventura, Josef Hron, Gyula M. Szabó, Amanda I. Karakas, Reto Trappitsch, Claudio B. Pereira, Larry R. Nittler, Maria Schönbächler, Marco Pignatari, Mattias Ek, B. Cseh, Maria Lugaro, A. Tattersall
Publikováno v:
The Astrophysical Journal
Stardust grains that originated in ancient stars and supernovae are recovered from meteorites and carry the detailed composition of their astronomical sites of origin. We present evidence that the majority of large ($\mu$m-sized) meteoritic silicon c
Publikováno v:
Astrophysical Journal; 8/20/2015, Vol. 809 Issue 2, p1-1, 1p