Key aspects in the photometric monitoring of δ Sct stars

Details Key aspects in the photometric monitoring of δ Sct stars Key aspects in the photometric monitoring of δ Sct stars

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000mons.proc...85p&link_type=abstract

The Third MONS Workshop: Science Preparation and Target Selection, Proceedings of a Workshop held in Aarhus, Denmark, January 24

Mathematics

Logic

Scientific paper

The MONS experiment will be able to verify some of the most important topics in the asteroseismologic studies of δ Sct stars. This research will benefit not only from the large increase in the number of detected frequencies, but also from the possibility to perform mode identification by means of very precise two--colour photometry. To do that, an appropriate frequency resolution, comparable to or better than what is currently achieved by ground--based observations, is necessary and hence two runs are recommended. To avoid over-scheduling of the Main Camera, a possible combination of observations from the Main Camera and from the Star Trackers is proposed. As a result, two key-objects as FG Vir and BH Psc could be adequately monitored, affording the possibility to enter into details of amplitude variations. As a by-product, the same results could be obtained on two γ Dor stars.

Affiliated with

Also associated with

No associations

Rating

Key aspects in the photometric monitoring of δ Sct stars 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 Key aspects in the photometric monitoring of δ Sct stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Key aspects in the photometric monitoring of δ Sct stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1622017