منابع مشابه
Incidence of high-amplitude δ Scuti type variable stars
An order-of-magnitude estimate for the incidence of high-amplitude δ Scuti-type variable stars (HADS) in the δ Scuti area of the H-R diagram is calculated. Using a model for the stellar distribution in the Milky Way, we calculate the number of stars that are expected to fall in the δ Scuti area of the H-R diagram within the magnitude range and sky coverage of the ROTSE Survey for Variables I (R...
متن کاملAmplitude investigation of δ Scuti variables in open clusters
We report here the results of a statistical analysis of 28 δ Scuti stars from five open clusters, α Persei, Pleiades, Hyades, Praesepe and Coma. These δ Scuti variables, most of which are on the main sequence, tend to show a positive correlation between oscillation amplitude and absolute luminosity. No correlation is found between amplitude and effective temperature .
متن کاملKey Aspects in the Photometric Monitoring of Δ Sct Stars
The MONS experiment will be able to verify some of the most important topics in the asteroseismologic studies of δ Sct stars. This research will benefit not only from the large increase in the number of detected frequencies, but also from the possibility to perform mode identification by means of very precise two–colour photometry. To do that, an appropriate frequency resolution, comparable to ...
متن کاملHD 172189 : An eclipsing and spectroscopic binary with a δ Sct - type pulsating component in an open cluster
We present a study based on more than 2500 uvby–measurements collected on HD 172189, a new eclipsing binary system with a δ Sct-type pulsating component that belongs to the open cluster IC 4756. The great interest of this object lies in that three important characteristics coexist: cluster membership, binarity and pulsation. Its binarity and the δ Sct-type pulsations of one component were detec...
متن کاملHipparcos parallaxes and period-luminosity relations of high-amplitude δ Scuti stars
Hipparcos parallaxes of high–amplitude δ Scuti stars are used to derive a period–luminosity relation with a scatter of about ±0.1 mag, which is independent from photometric calibrations to absolute luminosities. Comparisonswith several P–L relations from the literature show satisfactory agreement, and all deviations from theHipparcosmean relation canbe explainedby uncertainties in the data avai...
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ژورنال
عنوان ژورنال: Communications in Asteroseismology
سال: 2007
ISSN: 1021-2043,1021-2043
DOI: 10.1553/cia145s40