A Detailed Analysis of the Milky Way Warp Based on Classical Cepheids
Classical Cepheids (CCs) are important probes for the large-scale warp structure of the Milky Way. Using Gaia Data Release 3 CCs, we establish an optimal time-dependent warp model, where the warp height increases with radius following a power law, the ...
Xiaoyue Zhou +5 more
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Concluding Henrietta Leavitt's Work on Classical Cepheids in the Magellanic System and Other Updates of the OGLE Collection of Variable Stars [PDF]
I. Soszyński +11 more
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ULTRA-LOW AMPLITUDE VARIABLES IN THE LARGE MAGELLANIC CLOUD—CLASSICAL CEPHEIDS, POP. II CEPHEIDS, RV TAU STARS, AND BINARY VARIABLES [PDF]
J. Robert Buchler +5 more
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Vaginal-perianal or vaginal-perineal compared with vaginal-rectal culture-based screening for Group B Streptococci (GBS) colonization during the third trimester of pregnancy: a systematic review and meta-analysis. [PDF]
Nadeau HCG +5 more
europepmc +1 more source
The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. VII. Classical Cepheids in the Small Magellanic Cloud [PDF]
I. Soszyński +8 more
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The Role of Next-Generation Sequencing (NGS) in the Management of Tuberculosis: Practical Review for Implementation in Routine. [PDF]
Beviere M +6 more
europepmc +1 more source
Helium-burning stars, in particular Cepheids, are especially difficult to model, as the choice of free parameters can greatly impact the shape of the blue loops—the part of the evolutionary track at which the instability strip is crossed.
O. Ziółkowska +5 more
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Spatial Age Distribution of Classical Cepheids in Spiral Galaxies: The Cases of M31 and M33
Classical Cepheids can be used as age indicators due to well-established period–age and period–age–color relations. G. De Somma et al. refined these relations by including a metallicity term and different mass–luminosity assumptions.
Giulia De Somma +7 more
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Information Dark Energy Can Resolve the Hubble Tension and Is Falsifiable by Experiment. [PDF]
Gough MP.
europepmc +1 more source
Period Changes of Mira Variables, RR Lyrae Stars, and Type II Cepheids [PDF]
H. A. Smith
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