A Twelve-year Photometric Study of Lower Main Stars in the Hyades Cluster

Details A Twelve-year Photometric Study of Lower Main Stars in the Hyades Cluster A Twelve-year Photometric Study of Lower Main Stars in the Hyades Cluster

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...184.0523r&link_type=abstract

American Astronomical Society, 184th AAS Meeting, #05.23; Bulletin of the American Astronomical Society, Vol. 26, p.866

Astronomy and Astrophysics

Astronomy

Scientific paper

Between late 1980 and early 1992, we obtained differential Stromgren b and y photometric observations of 13 Hyades stars, spectral types F5V to K4V. The observations achieved and sustained millimagnitude precision. All ten G and K-type stars in the sample showed variability on time scales ranging from days to years. Rotational modulation proved to be a prominent and persistent component of the variation of these stars on the seasonal time scale. Correlated brightness and b-y color variations were found from year to year. There was, however, no significant correlation seen between the amplitudes of intraseasonal and interseasonal variability.

Affiliated with

Also associated with

No associations

Rating

A Twelve-year Photometric Study of Lower Main Stars in the Hyades Cluster 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 A Twelve-year Photometric Study of Lower Main Stars in the Hyades Cluster, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Twelve-year Photometric Study of Lower Main Stars in the Hyades Cluster will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-880836