Links

Tools

Export citation

Search in Google Scholar

On a new method to estimate distance, reddening and metallicity of RR Lyrae stars using optical/near-infrared ($B$,$V$,$I$,$J$,$H$,$K$) mean magnitudes: $ω$ Centauri as a first test case

Journal article published in 2018 by G. Bono, G. Iannicola, V. F. Braga, I. Ferraro, P. B. Stetson, D. Magurno, N. Matsunaga, R. L. Beaton, R. Buonanno, B. Chaboyer, M. Dall'Ora, M. Fabrizio, G. Fiorentino, W. L. Freedman, C. K. Gilligan and other authors.
This paper was not found in any repository; the policy of its publisher is unknown or unclear.
This paper was not found in any repository; the policy of its publisher is unknown or unclear.

Full text: Unavailable

Question mark in circle
Preprint: policy unknown
Upload
Question mark in circle
Postprint: policy unknown
Upload
Question mark in circle
Published version: policy unknown
Upload
Beta version