The Cepheid distance to the Large Magellanic Cloud and NGC 4258 by the surface brightness technique and improved calibration of the cosmic distance scale-Reference-Cited by-同舟云学术

The Cepheid distance to the Large Magellanic Cloud and NGC 4258 by the surface brightness technique and improved calibration of the cosmic distance scale

Published:2008-10 Issue: Volume: Page:
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Di Benedetto G. P.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/390/4/1762/3034496/mnras0390-1762.pdf

Reference44 articles.

1. The Distances to Open Clusters from Main‐Sequence Fitting. III. Improved Accuracy with Empirically Calibrated Isochrones

2. Über eine Möglichkeit, die Pulsationstheorie der δ Cephei-Veränderlichen zu prüfen

3. Stellar Angular Diameters and Visual Surface Brightness -- I LATE SPECTRAL TYPES

4. Infrared Surface Brightness Distances to Cepheids: A Comparison of Bayesian and Linear‐Bisector Calculations

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