Add to ORKGWe describe the search for delta Scuti stars in the MACHO database of bulge fields. Concentrating on a sample of high amplitude delta Scutis, we examine the light curves and pulsation modes. We also discuss their spatial distribution and evolutionary status using mean colors and absolute magnitudes
The MACHO Project database was searched for aperiodic blue variables in the LMC. Of approximately 25...
A general review of the pulsating {delta} Scuti variables is given including the observed light curv...
The purpose of asteroseismology is not only to derive the internal structure of individual stars fro...
The authors describe the search for {delta} Scuti stars in the MACHO database of bulge fields. Conce...
We have detected 90 objects with periods and lightcurve structure similar to those of field {delta} ...
The MACHO Project has been monitoring large fields in the direction of the Galactic bulge, the LMC a...
Abstract. Searching for main-sequence pulsators, we analyzed photometry of ∼200,000 variable star ca...
We present statistical characteristics of 1578 δ Scuti stars including nearby field stars and cluste...
We present an analysis on the behaviour of the Galactic bulge and the Large Magellanic Cloud (LMC) δ...
International audienceWe have made an asteroseismic analysis of the variable blue stragglers in the ...
The Praesepe cluster contains a number of δ Sct and γ Dor pulsators. Asteroseismology of cluster sta...
We review the pulsating stars contained in the top 24 fields of the MACHO bulge database, with speci...
Thanks to relatively firm mode identification, possible based on period ratios only, High Amplitude ...
With recent advances in CCD technology, it has become possible to detect low-amplitude variability i...
We present an analysis on the behaviour of the Galactic bulge and the Large Magellanic Cloud (LMC) δ...
The MACHO Project database was searched for aperiodic blue variables in the LMC. Of approximately 25...
A general review of the pulsating {delta} Scuti variables is given including the observed light curv...
The purpose of asteroseismology is not only to derive the internal structure of individual stars fro...
The authors describe the search for {delta} Scuti stars in the MACHO database of bulge fields. Conce...
We have detected 90 objects with periods and lightcurve structure similar to those of field {delta} ...
The MACHO Project has been monitoring large fields in the direction of the Galactic bulge, the LMC a...
Abstract. Searching for main-sequence pulsators, we analyzed photometry of ∼200,000 variable star ca...
We present statistical characteristics of 1578 δ Scuti stars including nearby field stars and cluste...
We present an analysis on the behaviour of the Galactic bulge and the Large Magellanic Cloud (LMC) δ...
International audienceWe have made an asteroseismic analysis of the variable blue stragglers in the ...
The Praesepe cluster contains a number of δ Sct and γ Dor pulsators. Asteroseismology of cluster sta...
We review the pulsating stars contained in the top 24 fields of the MACHO bulge database, with speci...
Thanks to relatively firm mode identification, possible based on period ratios only, High Amplitude ...
With recent advances in CCD technology, it has become possible to detect low-amplitude variability i...
We present an analysis on the behaviour of the Galactic bulge and the Large Magellanic Cloud (LMC) δ...
The MACHO Project database was searched for aperiodic blue variables in the LMC. Of approximately 25...
A general review of the pulsating {delta} Scuti variables is given including the observed light curv...
The purpose of asteroseismology is not only to derive the internal structure of individual stars fro...