The Faint Population in Baade's Window - Cycle 1

Details The Faint Population in Baade's Window - Cycle 1 The Faint Population in Baade's Window - Cycle 1

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1281k&link_type=abstract

HST Proposal ID #1281

Other

Hst Proposal Id #1281

Scientific paper

With 1500 sec in each of U, B, and V, at f/96, we will easily reach the main-sequence turnoff in the central bulge of the Milky Way, taking advantage of the low absorption in Baade's Window. FOC resolving power is adequate to separate stars down to the limited magnitude of ST. A by-product of another program will be a pair of V and I parallel WFC exposures, overlapping the same field.

Affiliated with

Also associated with

No associations

Rating

The Faint Population in Baade's Window - Cycle 1 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 The Faint Population in Baade's Window - Cycle 1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Faint Population in Baade's Window - Cycle 1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-862403