Hydrostatic evolutionary sequences for the nuclei of planetary nebulae
Copyright policy ) P. R. Wood; D. J. Faulkner;
Hydrostatic evolutionary sequences for the nuclei of planetary nebulae
Etude des proprietes des noyaux en fonction des trois parametres suivants: la masse du noyau, choisie egale a 0,60-0,70-0,76-0,89 MO; la phase de separation d'avec la branche asymptotique des geantes, choisie en quatre points egalement separes a l'interieur du cycle des flashes de l'helium; et la perte de masse qui prend toute une serie de formes
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These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
Citations provided by BIP!popularityPopularity provided by BIP!
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
Popularity provided by BIP! 162
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