Results 111 to 120 of about 577 (218)
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
Evolutionary tracks for 2–8 M _⊙ models, covering a [Fe/H] = −1.0 ( Z = 0.0014) to [Fe/H] = +0.2 ( Z = 0.02) metallicity range, are computed with Modules for Experiments in Stellar Astrophysics, MESA , to investigate evolutionary and pulsation properties
Radoslaw Smolec +4 more
doaj +1 more source
Variable stars toward the bulge of M 31: the AGAPE catalogue [PDF]
journal articleWe present the AGAPE astrometric and photometric catalogue of 1579 variable stars in a 14\u27 × 10\u27 field centred on M 31. This work is the first survey devoted to variable stars in the bulge of M 31. The R magnitudes of the objects and
Gondolo, Paolo +1 more
core
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
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
We report the discovery of LAMOST J0041+3948, the most luminous post-asymptotic giant-branch (AGB) Type II Cepheid known, located in the Andromeda Giant Stellar Stream.
Pinjian Chen +9 more
doaj +1 more source
Information Dark Energy Can Resolve the Hubble Tension and Is Falsifiable by Experiment. [PDF]
Gough MP.
europepmc +1 more source
The dynamics of variable stars
Harmonics, pulsation amplitude, and vibratory motion of Cepheid variable ...
Christy, R. F.
core
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

