Phase-dependent Variation of the Fundamental Parameters of Cepheids. III. Periods between 3 and 6 Days-Reference-Cited by-同舟云学术

Phase-dependent Variation of the Fundamental Parameters of Cepheids. III. Periods between 3 and 6 Days

Published:2005-10 Issue:4 Volume:130 Page:1880-1889
ISSN:0004-6256
Container-title:The Astronomical Journal
language:en
Short-container-title:Astron J

Author:

Andrievsky S. M.,Luck R. E.,Kovtyukh V. V.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference14 articles.

1. Magellanic Clouds elemental abundances from F supergiants: Revisited results for the Large Magellanic Cloud

2. The Galactic abundance gradient from Cepheids

3. Using Cepheids to determine the galactic abundance gradient

4. Berdnikov, L. N. & Ignatova, V. V. 2000, in ASP Conf. Ser. 203, The Impact of Large-Scale Surveys on Pulsating Star Research, ed. L. Szabados & D. W. Kurtz (San Francisco: ASP), 244

5. Galazutdinov, G. A. 1992, Preprints SAO Russian Acad. Sci., 92

Cited by 49 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Astrophysical calibration of the oscillator strengths of YJ-band absorption lines in classical Cepheids;Monthly Notices of the Royal Astronomical Society;2024-07-09

2. Cepheids as distance indicators and stellar tracers;The Astronomy and Astrophysics Review;2024-04-29

3. Effective temperatures of classical Cepheids from line-depth ratios in the H-band;Monthly Notices of the Royal Astronomical Society;2023-06-07

4. New Version of the Pulsating Photospheres Method: Multiphase Temprature Measurements of Cepheids;Astrophysical Bulletin;2022-06

5. A new and Homogeneous metallicity scale for Galactic classical Cepheids;Astronomy & Astrophysics;2022-05