BVRI light curves of KIC Cepheids (Szabo+, 2011)

Details BVRI light curves of KIC Cepheids (Szabo+, 2011) BVRI light curves of KIC Cepheids (Szabo+, 2011)

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74132709s&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/413/2709. Originally published in: 2011MNRAS.413.2709S

Other

Stars: Variable, Photometry: Ubvri

Scientific paper

We report results of initial work done on selected candidate Cepheids to be observed with the Kepler space telescope. Prior to the launch, 40 candidates were selected from previous surveys and data bases. The analysis of the first 322d of Kepler photometry, and recent ground-based follow-up multicolour photometry and spectroscopy allowed us to confirm that one of these stars, V1154 Cyg (KIC 7548061), is indeed a 4.9d Cepheid. Using the phase lag method, we show that this star pulsates in the fundamental mode. New radial velocity data are consistent with previous measurements, suggesting that a long-period binary component is unlikely. No evidence is seen in the ultraprecise, nearly uninterrupted Kepler photometry for non-radial or stochastically excited modes at the micromagnitude level. The other candidates are not Cepheids, but an interesting mix of possible spotted stars, eclipsing systems and flare stars.
(5 data files).

Affiliated with

Also associated with

No associations

Rating

BVRI light curves of KIC Cepheids (Szabo+, 2011) 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 BVRI light curves of KIC Cepheids (Szabo+, 2011), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and BVRI light curves of KIC Cepheids (Szabo+, 2011) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1565334