BV light curves of V511 Lyr in 1994-1996 (Lyytinen+, 2002)

Details BV light curves of V511 Lyr in 1994-1996 (Lyytinen+, 2002) BV light curves of V511 Lyr in 1994-1996 (Lyytinen+, 2002)

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33830197l&link_type=abstract

VizieR On-line Data Catalog: J/A+A/383/197. Originally published in: 2002A&A...383..197L

Computer Science

Stars: Variable, Stars: Double And Multiple, Photometry: Ubv

Scientific paper

Our time series analysis of sixteen BV light curves of the chromospherically active binary V511 Lyr confirmed the 2.7days rotation period uniquely. The seasonal periodicity changes of 3.8% indicated the presence of detectable surface differential rotation. The significant 2.67455days periodicity in the light curve minimum epochs suggested that the strongest starspot formation in V511 Lyr was concentrated on one stable active longitude. The differential BV photometry of V511 Lyr was made between May 1994 and June 1996 with the Vanderbilt-Tennessee State 0.4m Automated Photoelectric Telescope (APT). The comparison and check stars were HDE 337663 (C1) and HD 179422 (C2). (1 data file).

Affiliated with

Also associated with

No associations

Rating

BV light curves of V511 Lyr in 1994-1996 (Lyytinen+, 2002) 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 BV light curves of V511 Lyr in 1994-1996 (Lyytinen+, 2002), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and BV light curves of V511 Lyr in 1994-1996 (Lyytinen+, 2002) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1045119