CCD photometry of CY Aquarii IV. The 2012-2015 seasons

Research output: Contribution to journalArticle

Abstract

Based on more than 50 partial nights of CCD monitoring, we derive 118 new times of maximum light of the SX Phoenicis star CY Aquarii. These times support a linear ephemeris for 2013-2015.
Original languageEnglish
Pages (from-to)1-9
Number of pages9
JournalThe Journal of Astronomical Data
Volume22
Issue number1
Publication statusPublished - 1 Oct 2016

Keywords

  • technique: photometric
  • stars: individual: CY Aqr
  • variable stars: period change

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