Results 91 to 100 of about 4,708,970 (236)
Classification of Periodic Variable Stars from TESS
The number of known periodic variable stars has increased rapidly in recent years. As an all-sky transit survey, the Transiting Exoplanet Survey Satellite (TESS) plays an important role in detecting low-amplitude variable stars.
Xinyi Gao +3 more
doaj +1 more source
New Cepheid variables in the young open clusters Berkeley 51 and Berkeley 55 [PDF]
M. E. Lohr +5 more
openalex +1 more source
Pulsating Star Mystery Solved in Rare Alignment of Cepheid Variable and another Star [PDF]
. .
openalex +1 more source
The MACHO Project Large Magellanic Cloud Variable Star Inventory. XII. Three Cepheid Variables in Eclipsing Binaries [PDF]
C. Alcock +23 more
openalex +1 more source
Type II Cepheids: period-luminosity-metallicity relations for the Population II distance scale
Type II Cepheids are a class of pulsating variable stars that play a critical role in our understanding of stellar evolution, distance measurement and tracing the structure and kinematics of old stars in nearby galaxies.
Susmita Das +4 more
doaj +1 more source
The Orbit and Mass of the Cepheid AW Per
The Cepheid AW Per is a component in a multiple system with a long-period orbit. The radial velocities of Griffin cover the 38 yr orbit well. An extensive program of interferometry with the Center for High Angular Resolution Astronomy array is reported ...
Nancy Remage Evans +19 more
doaj +1 more source
Classical Cepheids (CCs) in Galactic open clusters (OCs) provide essential observational constraints for calibrating the period–age relation (PAR) and the period–Wesenheit relation (PWR) of CCs. However, distant and long-period OC Cepheids remain limited,
Shunhong Deng +9 more
doaj +1 more source
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
doaj +1 more source
Relation between Temperature and Radius in the Cepheid Variables [PDF]
A. E. H. Bleksley
openalex +1 more source
Crater II (CraII) is a very intriguing low surface brightness and extended galaxy in the vicinity of our Galaxy. Motivated by its huge area and the number of RR Lyrae stars (RRLSs) detected near to its core, we performed a follow-up campaign to get deep ...
A. Katherina Vivas +7 more
doaj +1 more source

