Abstract
Through time-series CCD photometry using a 155mm refractor, we found a new <TEX>$\delta$</TEX> Scuti type variable star, HD 235428, near a known bright <TEX>$\delta$</TEX> Scuti type star, DQ Cep. We performed follow-up observations using a 61cm telescope at Sobaeksan Optical Astronomy Observatory. Four frequencies have been derived by multiple-frequency analysis, which are 15.804, 5.498, 15.351 and 24.516cycle <TEX>$day^{-1}$</TEX>, respectively. V-amplitude of HD 235428 is <TEX>${\Delta} V$</TEX> = 0.026.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
