Results 81 to 90 of about 5,513 (166)
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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Relation between Temperature and Radius in the Cepheid Variables [PDF]
A. E. H. Bleksley
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The Gaia Parallax Discrepancy for the Cluster Pismis 19 and Separating δ Scutis from Cepheids
Pre-Gaia distances for the open cluster Pismis 19 disagree with Gaia parallaxes. A Two Micron All Sky Survey (2MASS) JK _s red clump distance was therefore established for Pismis 19 (2.90 ± 0.15 kpc), which reaffirms that zero-point corrections for Gaia ...
Daniel Majaess +12 more
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The Hubble Tension, a >5 σ discrepancy between direct and indirect measurements of the Hubble constant ( H _0 ), has persisted for a decade and motivated intense scrutiny of the paths used to infer H _0 .
Siyang Li +9 more
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A complete photometric study of the open cluster NGC 7790 containing Cepheid variables [PDF]
A. C. Gupta +3 more
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V725 Sagittarii: From Population II Cepheid to Red Semiregular Variable [PDF]
John R. Percy +5 more
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The geometry and distance of the Magellanic Clouds from Cepheid variables [PDF]
J. Caldwell, I. M. Coulson
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The MACHO Project LMC Variable Star Inventory. VIII. The Recent Star Formation History of the Large Magellanic Cloud from the Cepheid Period Distribution [PDF]
C. Alcock +22 more
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Ultra-long-period Cepheids as Standard Candles from Gaia to Rubin-LSST
An analysis of the properties of ultra-long-period Cepheids (ULPs) could significantly contribute to understanding the Hubble constant tension, e.g., the current discrepancy between determinations based on local distance indicators and those relying on ...
Ilaria Musella +12 more
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