King, Augmentation, Stellar Populations, Part 2

Details King, Augmentation, Stellar Populations, Part 2 King, Augmentation, Stellar Populations, Part 2

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4951k&link_type=abstract

HST Proposal ID #4951

Other

Hst Proposal Id #4951

Scientific paper

This proposal is a followup to the UV imaging in 3218, which discovered a UV and visible counterpart to the X-ray burster in NGC 6624. With the HSP, using a wide band in the UV, a 30-min data stream will be taken at the highest available rate, and two 40-min streams at about 300 mu-sec. The data will be analyzed over the known 11-minute binary orbit, the 30-40 Hz QPO range, and the 5 mu-sec period of a neighboring pulsar which may fall in the field of view. The S/N will be high enough to search for any other possible periodicities. The WFC will do parallel imaging at the edge of the cluster, in V and I.

Affiliated with

Also associated with

No associations

Rating

King, Augmentation, Stellar Populations, Part 2 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 King, Augmentation, Stellar Populations, Part 2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and King, Augmentation, Stellar Populations, Part 2 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1071732