A first-overtone RR Lyrae star with cyclic period changes
Open Access
- 1 November 2004
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 354 (3) , 821-826
- https://doi.org/10.1111/j.1365-2966.2004.08242.x
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This publication has 22 references indexed in Scilit:
- No evidence of a strong magnetic field in the Blazhko star RR LyraeAstronomy & Astrophysics, 2004
- The MACHO Project Large Magellanic Cloud Variable-Star Inventory. XIII. Fourier Parameters for the First-Overtone RR Lyrae Variables and the LMC DistanceThe Astronomical Journal, 2004
- Localizing the Solar Cycle Frequency Shifts in Globalp‐ModesThe Astrophysical Journal, 2002
- String/Rope length methods using the Lafler-Kinman statisticAstronomy & Astrophysics, 2002
- Period Changes in ω Centauri RR Lyrae StarsThe Astronomical Journal, 2001
- The MACHO Project Large Magellanic Cloud Variable‐Star Inventory. IX. Frequency Analysis of the First‐Overtone RR Lyrae Stars and the Indication for Nonradial PulsationsThe Astrophysical Journal, 2000
- Theoretical Period Changes in Yellow Giant PulsatorsThe Astrophysical Journal, 1998
- Is the Large Magellanic Cloud Microlensing Due to an Intervening Dwarf Galaxy?The Astrophysical Journal, 1997
- The Telescope System of the MACHO ProgramPublications of the Astronomical Society of the Pacific, 1996
- Mitteilung über veränderliche SterneAstronomische Nachrichten, 1907