METAL ABUNDANCES, RADIAL VELOCITIES, AND OTHER PHYSICAL CHARACTERISTICS FOR THE RR LYRAE STARS IN THEKEPLERFIELD-Reference-Cited by-同舟云学术

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METAL ABUNDANCES, RADIAL VELOCITIES, AND OTHER PHYSICAL CHARACTERISTICS FOR THE RR LYRAE STARS IN THEKEPLERFIELD

Published:2013-08-06 Issue:2 Volume:773 Page:181
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Nemec James M.,Cohen Judith G.,Ripepi Vincenzo,Derekas Aliz,Moskalik Pawel,Sesar Branimir,Chadid Merieme,Bruntt Hans

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/773/i=2/a=181/pdf

Reference141 articles.

1. The RR Lyrae Population of the Galactic Bulge from the MACHO Database: Mean Colors and Magnitudes

2. The MACHO Project Large Magellanic Cloud Variable‐Star Inventory. IX. Frequency Analysis of the First‐Overtone RR Lyrae Stars and the Indication for Nonradial Pulsations

3. The MACHO Project Large Magellanic Cloud Variable-Star Inventory. XIII. Fourier Parameters for the First-Overtone RR Lyrae Variables and the LMC Distance

4. The MACHO Project Large Magellanic Cloud Variable Star Inventory. XI. Frequency Analysis of the Fundamental‐Mode RR Lyrae Stars

5. Color-magnitude diagrams for seven globular clusters.

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3. The Next Generation Virgo Cluster Survey. XXXVII. Distant RR Lyrae Stars and the Milky Way Stellar Halo Out to 300 kpc;The Astrophysical Journal;2024-05-01

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5. Double-mode RR Lyrae stars observed by K2: analysis of high-precision Kepler photometry;Monthly Notices of the Royal Astronomical Society;2024-02-10

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