Results 91 to 100 of about 995 (187)
RW Arietis; an RR Lyrae Variable Star in an Eclipsing System [PDF]
W. Z. Wisniewski
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Pulsating stars are universally recognized as precise distance indicators and tracers of stellar populations. Their variability, combined with well-defined relationships between pulsation properties and intrinsic evolutionary parameters such as ...
Giulia De Somma +3 more
doaj +1 more source
Does the RR Lyrae variable DY And show the Blazhko effect? [PDF]
Z. Cano, Robert Connon Smith
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RR Lyrae Variables in M31 and M33
The properties of RR Lyrae variables make them excellent probes of the formation and evolution of a stellar population. The mere presence of such stars necessitates an age greater than ~10 Gyr while their periods and amplitudes can be used to estimate the metal abundance of the cluster or galaxy in which they reside.
openaire +2 more sources
RR Lyrae Variables in Local Group Galaxies: M31 [PDF]
G. Clementini +5 more
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This work is part of VESTALE, a project initiated within the Legacy Survey of Space and Time (LSST) Cadence Strategy Optimization Process. Its goal is to explore the potential of Rubin-LSST observations aimed at the Galactic bulge (henceforth just “Bulge”
M. Di Criscienzo +18 more
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On the Production of Bright RR Lyrae Variables in Metal-Rich Globular\n Clusters [PDF]
A. V. Sweigart, M. Catelan
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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
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Extended Stellar Populations in Ultrafaint Dwarf Galaxies
The possible existence of stellar halos in low-mass galaxies is being intensely discussed nowadays after some recent discoveries of stars located in the outskirts of dwarf galaxies of the Local Group.
Elisa A. Tau +2 more
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