Results 111 to 120 of about 5,915 (202)
The OGLE Collection of Variable Stars. Anomalous Cepheids in the Magellanic Clouds
18 pages, 9 figures, submitted to Acta ...
Soszynski, I. +12 more
openaire +2 more sources
Analysis of pulsating variable stars using the visibility graph algorithm. [PDF]
Muñoz V, Garcés NE.
europepmc +1 more source
The Period Radius Relation for Cepheid Variable Stars [PDF]
R. Woolley, B. Carter
openaire +1 more source
Modern tools for modeling stellar evolution, such as the Modules for Experiments in Stellar Astrophysics, offer state-of-the-art implementations of stellar theories.
O. Ziółkowska +4 more
doaj +1 more source
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
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
The OGLE Collection of Variable Stars. Classical Cepheids in the Magellanic System
16 pages, 5 ...
Soszynski, I. +12 more
openaire +2 more sources
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
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
Square root two period ratios in Cepheid and RR Lyrae variable stars
We document the presence of a few Cepheid and RR Lyrae variable stars with previously unrecognized characteristics. These stars exhibit the property of a period ratio of main pulsation divided by secondary pulsation P1/P2 very close to sqrt(2). Other stars of these types have period ratios which do not show clustering with a close association and a ...
Hippke, Michael +2 more
openaire +2 more sources

