Abstract
V1851 Orion (V1851 Ori) is an eclipsing binary star which an orbital period of 0.27695 days. We use the 0.5 - meter reflecting telescope and CCD with the standard visual (V) and red (R) filters of the UBV system at the Regional Obser-vatory for the Public, Chachoengsao, Thailand, to observe their light curve. The photometry method calculates the light curves construction and the time of minimum determination. In this work, the time minimum of V1851 Ori is HJD 2458105.0490. The period change is calculated using the O-C diagram and it is shown that the period of the V1851 Ori is decreasing which the rate of 2 × (-6.75647 × 10-12) day/cycle. That means the period reduces continuously by approximately 1.54 × 10-3 seconds/year.
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 callMore From: ASEAN Journal of Scientific and Technological Reports
Disclaimer: 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.
