Abstract We present new and accurate near-infrared J- and Ks-band data of the Large Magellanic Cloud cluster Reticulum. Data were collected with SOFI at the New Technology Telescope and covered an area of approximately 5'×5' around the center of the cluster. Current data allowed us to derive accurate mean K-band magnitudes for 21 fundamental (RRab) and 9 first-overtone (RRc) RR Lyrae stars. On the basis of the semiempirical K-band period-luminosity-metallicity (PLZK) relation we have recently derived, we find that the absolute distance to this cluster is 18.52+/-0.005 (random) +/-0.117 (systematic). Note that the current error budget is dominated by systematic uncertainty affecting the absolute zero-point calibration and the metallicity scale.

Dall'Ora, M., Storm, J., Bono, G., Ripepi, V., Monelli, M., Testa, V., et al. (2004). The Distance to the Large Magellanic Cloud Cluster Reticulum from the K-Band Period-Luminosity-Metallicity Relation of RR Lyrae Stars. THE ASTROPHYSICAL JOURNAL, 610(1), 269-274.

The Distance to the Large Magellanic Cloud Cluster Reticulum from the K-Band Period-Luminosity-Metallicity Relation of RR Lyrae Stars

BONO, GIUSEPPE;BUONANNO, ROBERTO;
2004-07-01

Abstract

Abstract We present new and accurate near-infrared J- and Ks-band data of the Large Magellanic Cloud cluster Reticulum. Data were collected with SOFI at the New Technology Telescope and covered an area of approximately 5'×5' around the center of the cluster. Current data allowed us to derive accurate mean K-band magnitudes for 21 fundamental (RRab) and 9 first-overtone (RRc) RR Lyrae stars. On the basis of the semiempirical K-band period-luminosity-metallicity (PLZK) relation we have recently derived, we find that the absolute distance to this cluster is 18.52+/-0.005 (random) +/-0.117 (systematic). Note that the current error budget is dominated by systematic uncertainty affecting the absolute zero-point calibration and the metallicity scale.
lug-2004
Pubblicato
Rilevanza internazionale
Articolo
Sì, ma tipo non specificato
Settore FIS/05 - ASTRONOMIA E ASTROFISICA
English
Con Impact Factor ISI
Stars: Evolution, Stars: Oscillations, Stars: Variables: Other
http://iopscience.iop.org/0004-637X/610/1/269/pdf/17951.web.pdf
Dall'Ora, M., Storm, J., Bono, G., Ripepi, V., Monelli, M., Testa, V., et al. (2004). The Distance to the Large Magellanic Cloud Cluster Reticulum from the K-Band Period-Luminosity-Metallicity Relation of RR Lyrae Stars. THE ASTROPHYSICAL JOURNAL, 610(1), 269-274.
Dall'Ora, M; Storm, J; Bono, G; Ripepi, V; Monelli, M; Testa, V; Andreuzzi, G; Buonanno, R; Caputo, F; Castellani, V; Corsi, Ce; Marconi, G; Marconi, M; Pulone, L; Stetson, Pb
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/52282
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