On The Distance Of The Globular Cluster M4 (NGC 6121) Using RR Lyrae Stars. I. Optical And Near-Infrared Period-Luminosity And Period-Wesenheit Relations

V. F. Braga, M. Dall'ora, G. Bono, P. B. Stetson, I. Ferraro, G. Iannicola, M. Marengo, J. Neeley, S. E. Persson, R. Buonanno, G. Coppola, W. Freedman, B. F. Madore, M. Marconi, N. Matsunaga, A. Monson, J. Rich, V. Scowcroft, M. Seibert

Research output: Contribution to journalArticle

48 Citations (Scopus)
Original languageEnglish
Pages (from-to)165
JournalAstrophysical Journal
Volume799
Issue number2
DOIs
Publication statusPublished - 2015

Cite this

Braga, V. F., Dall'ora, M., Bono, G., Stetson, P. B., Ferraro, I., Iannicola, G., Marengo, M., Neeley, J., Persson, S. E., Buonanno, R., Coppola, G., Freedman, W., Madore, B. F., Marconi, M., Matsunaga, N., Monson, A., Rich, J., Scowcroft, V., & Seibert, M. (2015). On The Distance Of The Globular Cluster M4 (NGC 6121) Using RR Lyrae Stars. I. Optical And Near-Infrared Period-Luminosity And Period-Wesenheit Relations. Astrophysical Journal, 799(2), 165. https://doi.org/10.1088/0004-637X/799/2/165