THE ONSET OF CHAOS IN PULSATING VARIABLE STARS
Random changes in pulsation period occur in cool pulsating Mira variables, Type A, B, and C semiregular variables, RV Tauri variables, and in most classical Cepheids.
D. G. Turner +3 more
doaj +3 more sources
Little Bear's Pulsating Stars: Variable Star Census of dSph UMi Galaxy [PDF]
Recent observations and a photometric search for variable stars in the Ursa Minor dwarf spheroidal galaxy (UMi dSph) are presented. Our observations were taken at Apache Point Observatory in 2014 and 2016 using the 0.5m ARCSAT telescope and the West Mountain Observatory 0.9m telescope of Brigham Young University in 2016. Previously known RR Lyrae stars
Karen Kinemuchi +4 more
openalex +3 more sources
PULSATING VARIABLE STARS IN THE COMA BERENICES DWARF SPHEROIDAL GALAXY [PDF]
14 pages, 3 figures, Accepted for publication in ...
I. Musella +10 more
openalex +4 more sources
Pulsating variable stars in the Magellanic Clouds [PDF]
AbstractPulsating variable stars can be powerful tools to study the structure, formation and evolution of galaxies. I discuss the role that the Magellanic Clouds' pulsating variables play in our understanding of the whole Magellanic System, in light of results on pulsating variables produced by extensive observing campaigns like the MACHO and OGLE ...
Gisella Clementini
openalex +3 more sources
Pulsating Variable Stars in the MACHO Bulge database: The Semiregular Variables [PDF]
We review the pulsating stars contained in the top 24 fields of the MACHO bulge database, with special emphasis on the red semiregular stars. Based on period, amplitude and color cuts, we have selected a sample of 2000 semiregular variables with ...
D. Minniti +19 more
+6 more sources
Little Bear’s pulsating stars: Variable star census of UMi dSph Galaxy [PDF]
Recent observations and a photometric search for variable stars in the Ursa Minor dwarf spheroidal galaxy (UMi dSph) are presented. Our observations were taken at Apache Point Observatory in 2014 and 2016 using the 0.5m ARCSAT telescope and the West Mountain Observatory (WMO) 0.9m telescope of Brigham Young University in 2016. Previously known RR Lyrae
Karen Kinemuchi +4 more
openalex +3 more sources
Pulsation models for the 0.26 M⊙ star mimicking RR Lyrae pulsator. Model survey for the new class of variable stars [PDF]
We present non-linear hydrodynamic pulsation models for OGLE-BLG-RRLYR-02792 - a 0.26M_sun pulsator, component of the eclipsing binary system, analysed recently by Pietrzynski et al. The star's light and radial velocity curves mimic that of classical RR Lyrae stars, except for the bump in the middle of the ascending branch of the radial velocity curve.
R. Smolec +13 more
openalex +6 more sources
Pulsating and variable stars in the young open star cluster NGC 6231
Diese Arbeit befasst sich mit den veränderlichen und im speziellen mit pulsierenden Sternen in NGC 6231, also Sternen die ü̈ber typische Zeiträume ihre Form und auch physikalischen Eigenschaften ändern. Obwohl sich schon einige Studien in den letzten 30 Jahren mit diesem Thema beschäftigt haben, fehlt immer noch ein vollständiges Bild von Pulsatoren in
Stefan Meingast
openalex +2 more sources
Observational Properties of 155 O- and B-type Massive Pulsating Stars
O- and B-type (OB-type) pulsating stars are important objects for studying the structure and evolution of massive stars through asteroseismology. A large amount of data from various sky surveys provides an unprecedented opportunity to search for and ...
Xiang-dong Shi +5 more
doaj +1 more source
Investigating Stellar Variability in the Open Cluster Region NGC 381
We study variable stars in the field of the open cluster NGC 381 using photometric data observed over 27 nights and identify a total of 57 variable stars, six of which are member stars. The variable stars are classified based on their periods, amplitudes,
Jayanand Maurya +3 more
doaj +1 more source

