The first spectroscopically confirmed Mira star in M33-Reference-Cited by-同舟云学术

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The first spectroscopically confirmed Mira star in M33

Published:2011-03-02 Issue:3 Volume:413 Page:1797-1802
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Barsukova E. A.,Goranskij V. P.,Hornoch K.,Fabrika S.,Pietsch W.,Sholukhova O.,Valeev A. F.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/413/3/1797/2882004/mnras0413-1797.pdf

Reference40 articles.

1. The SCORPIO universal focal reducer of the 6-m telescope

2. Visual Versus Near-Infrared Variability of R For: Evidence for a Multiperiodic Circumstellar Modulation

3. A note on bolometric corrections for late-type stars and long-period variables

4. The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33

Cited by 4 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. A Distance Measurement to M33 Using Optical Photometry of Mira Variables;The Astronomical Journal;2023-03-01

2. Near-infrared Mira Period–Luminosity Relations in M33;The Astronomical Journal;2018-08-20

3. The M33 Synoptic Stellar Survey. II. Mira Variables;The Astronomical Journal;2017-03-22

4. UBV photometry of X-ray system with M2 III type red giant V934 her (4U 1700+24);Astrophysical Bulletin;2012-01

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