Photometric Variability in the HR Diagram

Details Photometric Variability in the HR Diagram Photometric Variability in the HR Diagram

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997esasp.402..467e&link_type=abstract

Proceedings of the ESA Symposium `Hipparcos - Venice '97', 13-16 May, Venice, Italy, ESA SP-402 (July 1997), p. 467-472

Physics

39

Scientific paper

The Hipparcos satellite has detected systematically variable stars when the amplitudes exceed a magnitude dependent threshold, as small as a few millimag for bright stars. The published data about variable stars result from the work of two groups at the Geneva Observatory and at the Royal Greenwich Observatory. It contains information about periodic variables (extrema, periods and epochs) and about `unsolved' variables (amplitudes). Here, a more general description of the HR-diagram is made in terms of stability, microvariability, variability, and variation time scales. A particular emphasis is put on the limits of stability areas and their signification.

Affiliated with

Also associated with

No associations

Rating

Photometric Variability in the HR Diagram 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 Photometric Variability in the HR Diagram, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometric Variability in the HR Diagram will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1879291