On the Distance of the Sun from the Galactic Plane. [PDF]
Proc Natl Acad Sci U S A, 1927 Gerasimovic BP, Luyten WJ.
europepmc +1 more source
Note on the Problem of Great Stellar Distances. [PDF]
Proc Natl Acad Sci U S A, 1922 Shapley H.
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THE MAGELLANIC CLOUDS. XVI. INFRARED STARS AND STELLAR EVOLUTION. [PDF]
Proc Natl Acad Sci U S A, 1955 Shapley H.
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Galactic and Extragalactic Studies: I. On the Corona of Stars Around the Galactic System. [PDF]
Proc Natl Acad Sci U S A, 1939 Shapley H.
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A re-determination of the radial velocity curves of certain Cepheid variable stars
Lick Observatory Bulletins, 1926 openaire +2 more sources
The occurrence of carbon stars and Cepheid variables in common fields of the Magellanic Clouds
The Astrophysical Journal, 1982 openaire +1 more source
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A distance to the galaxy NGC4258 from observations of Cepheid variable stars
Nature, 1999Cepheid variable stars pulsate in a way that is correlated with their intrinsic luminosity, making them useful as 'standard candles' for determining distances to galaxies; the potential systematic uncertainties in the resulting distances have been estimated to be only 8-10%.
Maoz, Eyal +7 more
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Spectra of Population II Cepheid Variable Stars
1958The physical properties of the population II cepheids have been studied using the following material: photoelectric observations of Arp, low dispersion spectra of Joy, high dispersion spectra taken by Sanford and Abt, and numerous moderate dispersion spectra obtained by the author. Radial velocity curves for ten cepheids are shown.
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A New Approach to the Determination of the Intrintic Colours of the Cepheid Variable Stars
International Astronomical Union Colloquium, 1979SummaryIntrinsic colours have been determined for 247 of the 275 variable stars listed in the “Catalogue of the Light and Colour Curves of Cepheids in the UBV System” by N. Nikolov. Algorithms for computing intrinsic colour are derived from 59 standard stars.
Gerald E. Kron, Franklin E. Roach
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Domain Adaptation under Data Misalignment: An Application to Cepheid Variable Star Classification
2014 22nd International Conference on Pattern Recognition, 2014We address a particular scenario within the area of domain adaptation, where a predictive model obtained from a source domain can be applied directly to a target domain. Both source and target domains share the same input or feature space, but we do not impose any restrictions on the marginal and class posterior distributions (both distributions can ...
Ricardo Vilalta +2 more
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