On a new parameter to estimate the Helium content in old stellar systems

Troisi, F.; Bono, G.; Stetson, P. B.; Pietrinferni, A.; Weiss, A.; Fabrizio, M.; Ferraro, I.; Di Cecco, A.; Iannicola, G.; Buonanno, R.; Calamida, A.; Caputo, F.; Corsi, C. E.; Dall’Ora, M.; Kunder, A.; Monelli, M.; Nonino, M.; Piersimoni, A. M.; Pulone, L.; Romaniello, M.; Walker, A. R.; Zoccali, M.

doi:10.1086/661534

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On a new parameter to estimate the Helium content in old stellar systems

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Weiss, A.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Troisi, F., Bono, G., Stetson, P. B., Pietrinferni, A., Weiss, A., Fabrizio, M., et al. (2011). On a new parameter to estimate the Helium content in old stellar systems. Publications of the Astronomical Society of the Pacific, 123(906), 879-891. doi:10.1086/661534.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0012-2589-F

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