arXiv · 1812.03025
Investigating the population of Galactic star formation regions and star clusters within a Wide-Fast-Deep Coverage of the Galactic Plane
Abstract
One of the aims of LSST is to perform a systematic survey of star clusters and star forming regions (SFRs) in our Galaxy. In particular, the observations obtained with LSST will make a big difference in Galactic regions that have been poorly studied in the past, such as the anticenter and the disk beyond the Galactic center, and they will have a strong impact in discovering new distant SFRs. These results can be achieved by exploiting the exquisite depth that will be attained if the wide-fast-deep (WFD) observing strategy of the main survey is also adopted for the Galactic plane, in the g, r, and i filters.
Explore related subjects
Keep this discovery
L. Prisinzano, L. Magrini, F. Damiani, G. Sacco, R. Bonito, L. Venuti, G. Casali, V. Roccatagliata, S. Randich, L. Inno, T. Cantat-Gaudin, D. Minniti, A. Bragaglia, S. Degli Innocenti, P. G. Prada Moroni, E. Tognelli, A. Sollima, A. Vallenari, M. Guarcello, S. Messina, G. Micela, S. Sciortino, A. Spagna, N. Sanna, J. Kastner, A. Roman, R. Szabo, B. Dias, E. Feigelson, R. Jeffries, E. Friel, J. Stauffer, M. Van der Swaelmen, R. Sordo, D. Bossini. 2018-12-07. Investigating the population of Galactic star formation regions and star clusters within a Wide-Fast-Deep Coverage of the Galactic Plane. https://arxiv.org/abs/1812.03025
Cite the original work for its findings. Save a collection to share your selection of sources.