most citedOn the stellar content of the starburst galaxy IC10

22 citations · 25 across the 2 of their papers we have counts for

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astro-ph20083 cited

C/O white dwarfs of very low mass: 0.33-0.5 Mo

P. G. Prada Moroni, O. Straniero

The standard lower limit for the mass of white dwarfs (WDs) with a C/O core is roughly 0.5 Mo. In the present work we investigated the possibility to form C/O WDs with mass as low…

astro-ph200842 cited

On the distance and reddening of the starburst galaxy IC10

N. Sanna, G. Bono, P. B. Stetson +16

We present deep and accurate optical photometry of the Local Group starburst galaxy IC10. The photometry is based on two sets of images collected with the Advanced Camera for Surve…

astro-ph200740 cited

On the white dwarf cooling sequence of the globular cluster Omega Centauri

A. Calamida, C. E. Corsi, G. Bono +16

We present deep and precise photometry (F435, F625W, F658N) of Omega Cen collected with the Advanced Camera for Surveys (ACS) on board the Hubble Space Telescope (HST). We have ide…

astro-ph20079 cited

Microscopic Diffusion in Stellar Evolution Codes: First Comparison results of ESTA-Task~3

Y. Lebreton, J. Montalban, J. Christensen-Dalsgaard +8

We present recent work undertaken by the Evolution and Seismic Tools Activity (ESTA) team of the CoRoT Seismology Working Group. The new ESTA-Task 3 aims at testing, comparing and…

astro-ph200729 cited

White Dwarf cooling Sequences, II: luminosity functions

P. G. Prada Moroni, O. Straniero

Given the importance of white dwarfs (WDs) in many fields of modern astrophysics, the precise knowledge of the actual degree of accuracy of the associated theoretical predictions i…

astro-ph200699 cited

Recovering the star formation rate in the solar neighborhood

M. Cignoni, S. Degl'Innocenti, P. G. Prada Moroni +1

This paper develops a method for obtaining the star formation histories of a mixed, resolved population through the use of color-magnitude diagrams (CMDs). The method provides insi…