activity
20042008
most citedInter-comparison of the g-, f- and p-modes calculated using different oscillation codes for a given stellar model

38 citations · 76 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph20082 cited

Input from opacity data in computation of pulsation instability

Josefina Montalbán, Andrea Miglio

Several types of variable stars are found along the HR diagram whose pulsations are driven by the -mechanism. Given their nature, the precise () domain where thes…

astro-ph200738 cited

Inter-comparison of the g-, f- and p-modes calculated using different oscillation codes for a given stellar model

A. Moya, J. Christensen-Dalsgaard, S. Charpinet +9

In order to make astroseismology a powerful tool to explore stellar interiors, different numerical codes should give the same oscillation frequencies for the same input physics. Th…

astro-ph20076 cited

Close-up of primary and secondary asteroseismic CoRoT targets and the ground-based follow-up observations

K. Uytterhoeven, E. Poretti, M. Rainer +13

To optimise the science results of the asteroseismic part of the CoRoT satellite mission a complementary simultaneous ground-based observational campaign is organised for selected…

astro-ph200720 cited

12 Bootis: a test bed for extra-mixing processes in stars

Andrea Miglio, Josefina Montalban, Carla Maceroni

12 Bootis is a spectroscopic binary whose visual orbit has been resolved by interferometry. Though the physical parameters of the system have been determined with an excellent prec…

astro-ph20073 cited

A Splinter Session on the Thorny Problem of Stellar Ages

Eric E. Mamajek, David Barrado y Navascues, Sofia Randich +4

Accurate stellar ages remain one of the most poorly constrained, but most desired, astronomical quantities. Here we briefly summarize some recent efforts to improve the stellar age…

astro-ph20047 cited

Solar model with CNO revised abundances

J. Montalban, A. Miglio, A. Noels +3

Recent three-dimensional, NLTE analyses of the solar spectrum have shown a significant reduction in the C, N, O and Ne abundances leading to a Z/X ratio of the order of 0.0177. We…