Geneva photometry of HD 129929 (Aerts+, 2004)

Details Geneva photometry of HD 129929 (Aerts+, 2004) Geneva photometry of HD 129929 (Aerts+, 2004)

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..34150241a&link_type=abstract

VizieR On-line Data Catalog: J/A+A/415/241. Originally published in: 2004A&A...415..241A

Computer Science

Stars: Variable, Photometry: Geneva

Scientific paper

We have gathered and analysed a timeseries of 1493 high-quality multicolour Geneva photometric data of the B3V {beta} Cep star Hd 129929. The dataset has a time base of 21.2 years. The occurrence of a beating phenomenon is evident from the data. We find evidence for the presence of at least six frequencies, among which we see components of two frequency multiplets with an average spacing of ~0.0121c/d which points towards very slow rotation. This result is in agreement with new spectroscopic data of the star and also with previously taken UV spectra. We provide the amplitudes of the six frequencies in all seven photometric filters. The metal content of the star is Z=0.018+/-0.004. All these observational results will be used to perform detailed seismic modelling of this massive star in a subsequent paper.
(1 data file).

Affiliated with

Also associated with

No associations

Rating

Geneva photometry of HD 129929 (Aerts+, 2004) 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 Geneva photometry of HD 129929 (Aerts+, 2004), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Geneva photometry of HD 129929 (Aerts+, 2004) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1768786