Autor: |
Botan, E., Saito, R. K., Minniti, D., Kanaan, A., Ramos, R. Contreras, Ferreira, T. S., Gramajo, L. V., Navarro, M. G. |
Rok vydání: |
2021 |
Předmět: |
|
Druh dokumentu: |
Working Paper |
DOI: |
10.1093/mnras/stab888 |
Popis: |
Most of our knowledge about the structure of the Milky Way has come from the study of variable stars. Among the variables, mimicking the periodic variation of pulsating stars, are the eclipsing binaries. These stars are important in astrophysics because they allow us to directly measure radii and masses of the components, as well as the distance to the system, thus being useful in studies of Galactic structure alongside pulsating RR Lyrae and Cepheids. Using the distinguishing features of their light curves, one can identify them using a semi-automated process. In this work, we present a strategy to search for eclipsing variables in the inner VVV bulge across an area of 13.4 sq. deg. within $1.68^{\rm o}Comment: 14 pages. 12 figures. 3 tables. Accepted for publication in MNRAS |
Databáze: |
arXiv |
Externí odkaz: |
|