Results 61 to 70 of about 266 (162)
The OGLE Collection of Variable Stars. Classical Cepheids in the Magellanic System
16 pages, 5 ...
Soszynski, I. +12 more
openaire +2 more sources
We present a novel technique for mapping single-phase observations of Cepheids in any given band into their time-averaged values, using strong priors on the known interrelations of the multiwavelength widths of Cepheid period–luminosity (PL) relations ...
Barry F. Madore +2 more
doaj +1 more source
We present homogeneous, near-infrared ( JHK _s bands) time-series observations of the classical Carina dwarf spheroidal (dSph) galaxy to determine accurate and precise distances using the pulsating stars as standard candles.
Chow-Choong Ngeow +3 more
doaj +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
Analysis of pulsating variable stars using the visibility graph algorithm. [PDF]
Muñoz V, Garcés NE.
europepmc +1 more source
The OGLE Collection of Variable Stars. Type II Cepheids in the Magellanic System
BEFORE_PUBLICATION
Soszyński, Igor +12 more
openaire +3 more sources
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
The Period Radius Relation for Cepheid Variable Stars [PDF]
R. Woolley, B. Carter
openaire +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

