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of 1 433
pro vyhledávání: '"Forestini, M."'
We present a scenario to explain the lithium-rich phase which occurs on the red giant branch at the so-called bump in the luminosity function. The high transport coefficients required to enhance the surface lithium abundance are obtained in the frame
Externí odkaz:
http://arxiv.org/abs/astro-ph/0106441
Publikováno v:
Astron.Astrophys.358:593-599,2000
We present new grids of pre-main sequence (PMS) tracks for stars in the mass range 0.1 to 7.0 Msun. The computations were performed for four different metallicities (Z=0.01, 0.02, 0.03 and 0.04). A fifth table has been computed for the solar composit
Externí odkaz:
http://arxiv.org/abs/astro-ph/0003477
Nucleosynthesis in evolved (RGB and AGB) low-mass stars is reviewed under the light of the reaction rates recommended in the NACRE compilation (Angulo et al. 1999). We use a parametric model of stellar nucleosynthesis to investigate the uncertainties
Externí odkaz:
http://arxiv.org/abs/astro-ph/9910289
Publikováno v:
AIP Conference Proceedings; Feb1995, Vol. 327 Issue 1, p403-406, 4p
Publikováno v:
Scopus-Elsevier
NASA Astrophysics Data System
NASA Astrophysics Data System
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::1241bc24317f40b25fe330a95ca01bc1
http://hdl.handle.net/11391/8565
http://hdl.handle.net/11391/8565
Autor:
Paulus, G., Forestini, M.
Publikováno v:
AIP Conference Proceedings; Aug1991, Vol. 232 Issue 1, p183-189, 7p
Autor:
Battino, Umberto1 (AUTHOR) u.battino@hull.ac.uk, Roberti, Lorenzo2,3,4 (AUTHOR), Lawson, Thomas V.1,5 (AUTHOR), Laird, Alison M.6 (AUTHOR), Todd, Lewis6 (AUTHOR)
Publikováno v:
Universe (2218-1997). May2024, Vol. 10 Issue 5, p204. 14p.
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
6 pags., 4 figs.
Observations and stellar evolution computations have been dedicated to the search for 14C in the archetype of AGB stars, IRC+10216/CW Leo. Contrary to Wright’s (1994) tentative detection, we see no trace of 14CO in this star d
Observations and stellar evolution computations have been dedicated to the search for 14C in the archetype of AGB stars, IRC+10216/CW Leo. Contrary to Wright’s (1994) tentative detection, we see no trace of 14CO in this star d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::01e2207bac3b5a92484b46bee75b42ea
http://hdl.handle.net/10261/265588
http://hdl.handle.net/10261/265588
Publikováno v:
Space Science Reviews; 1993, Vol. 66 Issue 1-4, p409-412, 4p
Publikováno v:
Astronomy and Astrophysics; August 2001, Vol. 375 Issue: 1 pL9-L13, 5p