Crowded Fields in the Milky Way and Beyond

Details Crowded Fields in the Milky Way and Beyond Crowded Fields in the Milky Way and Beyond

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.576..637b&link_type=abstract

"Proceedings of the Gaia Symposium "The Three-Dimensional Universe with Gaia" (ESA SP-576). Held at the Observatoire de Paris-Me

Computer Science

Gaia, Simulations, Galaxy Bulge, Globular Clusters, Galaxies Local Group

Scientific paper

Although most of the sky will be almost empty to Gaia's high resolution eyes, several high density regions will be observed. They will present a challenge both for the onboard data handling and for the ground-based reduction, while being crucial for the Gaia science case. Indeed, the highest star densities are expected in the Galactic bulge low-extinction regions such as Baade's window, Galactic globular clusters and in the central regions of the Large Magellanic Cloud. I will present here those regions, their scientific impact and their observational complexity.

Affiliated with

Also associated with

No associations

Rating

Crowded Fields in the Milky Way and Beyond does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Crowded Fields in the Milky Way and Beyond, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Crowded Fields in the Milky Way and Beyond will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-899056