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Updated: May 23, 2026

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RR-Lyrae型の脈動は,二重星系にある太陽質量0.26の恒星からのものです

G Pietrzyński1, I B Thompson, W Gieren

  • 1Departamento de Astronomìa, Universidad de Concepción, Casilla 160-C, Concepciòn, Chile. pietrzyn@astrouw.edu.pl

Nature
|April 7, 2012
PubMed
まとめ

奇妙な RR Lyrae 星は,日食のバイナリ系にある低質量物体であることが判明しました. この発見は,珍しいものの,このような二重星系は真のRRライレー星を模倣し,恒星集団の研究に影響を与える可能性があることを示唆しています.

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