Polaris: History of Pulsation Activity since Discovery

Authors

  • I.O. Usenko Astronomical Observatory, Odessa National University, Research Institute «Mykolaiv Astronomical Observatory»
  • V.V. Kovtyukh Astronomical Observatory, Odessa National University
  • A.S. Miroshnichenko Department of Physics and Astronomy, University of North Carolina at Greensboro
  • S. Danford Department of Physics and Astronomy, University of North Carolina at Greensboro

DOI:

https://doi.org/10.15407/scine13.01.099

Keywords:

Cepheids, pulsation periods, radial velocities, stars, variable amplitude, α Umi

Abstract

The pulsation activity of small-amplitude Cepheid Alpha UMi (Polaris) during the period of its radial velocity observations has been analyzed. In the 20th century, Polaris was known to demonstrate a decrease in radial velocity amplitude to the minimum, in the 1980s. Thereafter, the amplitude has increased. The observations of September-December 2015 (21 spectra) obtained by 81cm telescope TCO with spectrograph have showed that radial velocity amplitude comes to 4.16 km/s and is approximately twice higher than the estimates made in 2007, with pulsation period adding 8.6 min.

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Published

2024-08-27

How to Cite

Usenko, I., Kovtyukh, V., Miroshnichenko, A., & Danford, S. (2024). Polaris: History of Pulsation Activity since Discovery. Science and Innovation, 13(1), 99–103. https://doi.org/10.15407/scine13.01.099

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Section

Scientific Framework of Innovation Activity