other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
2019ApJ...870..115B - Astrophys. J., 870, 115-115 (2019/January-2)
On a new method to estimate the 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.
BONO G., IANNICOLA G., BRAGA V.F., FERRARO I., STETSON P.B., MAGURNO D., MATSUNAGA N., BEATON R.L., BUONANNO R., CHABOYER B., DALL'ORA M., FABRIZIO M., FIORENTINO G., FREEDMAN W.L., GILLIGAN C.K., MADORE B.F., MARCONI M., MARENGO M., MARINONI S., MARRESE P.M., MARTINEZ-VAZQUEZ C.E., MATEO M., MONELLI M., NEELEY J.R., NONINO M., SNEDEN C., THEVENIN F., VALENTI E. and WALKER A.R.
Abstract (from CDS):
Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.
Journal keyword(s): globular clusters: individual: Centauri - stars: distances - stars: horizontal-branch - stars: variables: RR Lyrae
VizieR on-line data: <Available at CDS (J/ApJ/870/115): table1.dat>
Simbad objects: 174
To bookmark this query, right click on this link: simbad:2019ApJ...870..115B and select 'bookmark this link' or equivalent in the popup menu