Rujukan Gelung biru

  1. Pols, Onno (September 2009). "Chapter 9: Post-main sequence evolution through helium burning" (PDF). Stellar Structure and Evolution (lecture notes). Diarkibkan daripada yang asal (PDF) pada 2019-05-20. Dicapai pada 2019-01-17.
  2. Xu, H. Y.; Li, Y. (2004). "Blue loops of intermediate mass stars . I. CNO cycles and blue loops". Astronomy and Astrophysics. 418: 213–224. Bibcode:2004A&A...418..213X. doi:10.1051/0004-6361:20040024.
  3. Halabi, Ghina M.; El Eid, Mounib (2012). "Sensitivity of the blue loops of intermediate-mass stars to nuclear reactions". American Institute of Physics Conference Series. 1498 (1): 334. arXiv:1410.1652. Bibcode:2012AIPC.1498..334H. doi:10.1063/1.4768514. S2CID 7679927.
  4. 1 2 Groenewegen, M. A. T.; Jurkovic, M. I. (2017). "Luminosities and infrared excess in Type II and anomalous Cepheids in the Large and Small Magellanic Clouds". Astronomy and Astrophysics. 603: A70. arXiv:1705.00886. Bibcode:2017A&A...603A..70G. doi:10.1051/0004-6361/201730687. S2CID 118883548.
  5. Meynet, Georges; Georgy, Cyril; Hirschi, Raphael; Maeder, André; Massey, Phil; Przybilla, Norbert; Nieva, M. -Fernanda (2011). "Red Supergiants, Luminous Blue Variables and Wolf-Rayet stars: The single massive star perspective". Bulletin de la Société Royale des Sciences de Liège. 80: 266. arXiv:1101.5873. Bibcode:2011BSRSL..80..266M.
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