The authors describe the search for {delta} Scuti stars in the MACHO database of bulge fields. Concentrating on a sample of high amplitude {delta} Scutis, they examine the light curves and pulsation modes. They also discuss their spatial distribution and evolutionary status using mean colors and absolute magnitudes
Thanks to relatively firm mode identification, possible based on period ratios only, High Amplitude ...
We present the microlensing optical depth toward the Galactic bulge based on the detection of 99 eve...
The Chandra Galactic Bulge Survey (CGBS) is a shallow but wide survey of two approximately 6x1 degre...
We describe the search for delta Scuti stars in the MACHO database of bulge fields. Concentrating on...
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 an analysis on the behaviour of the Galactic bulge and the Large Magellanic Cloud (LMC) δ...
We review the pulsating stars contained in the top 24 fields of the MACHO bulge database, with speci...
We present statistical characteristics of 1578 δ Scuti stars including nearby field stars and cluste...
The MACHO Project database was searched for aperiodic blue variables in the LMC. Of approximately 25...
We present an analysis on the behaviour of the Galactic bulge and the Large Magellanic Cloud (LMC) δ...
With recent advances in CCD technology, it has become possible to detect low-amplitude variability i...
The Praesepe cluster contains a number of δ Sct and γ Dor pulsators. Asteroseismology of cluster sta...
International audienceWe have made an asteroseismic analysis of the variable blue stragglers in the ...
Thanks to relatively firm mode identification, possible based on period ratios only, High Amplitude ...
We present the microlensing optical depth toward the Galactic bulge based on the detection of 99 eve...
The Chandra Galactic Bulge Survey (CGBS) is a shallow but wide survey of two approximately 6x1 degre...
We describe the search for delta Scuti stars in the MACHO database of bulge fields. Concentrating on...
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 an analysis on the behaviour of the Galactic bulge and the Large Magellanic Cloud (LMC) δ...
We review the pulsating stars contained in the top 24 fields of the MACHO bulge database, with speci...
We present statistical characteristics of 1578 δ Scuti stars including nearby field stars and cluste...
The MACHO Project database was searched for aperiodic blue variables in the LMC. Of approximately 25...
We present an analysis on the behaviour of the Galactic bulge and the Large Magellanic Cloud (LMC) δ...
With recent advances in CCD technology, it has become possible to detect low-amplitude variability i...
The Praesepe cluster contains a number of δ Sct and γ Dor pulsators. Asteroseismology of cluster sta...
International audienceWe have made an asteroseismic analysis of the variable blue stragglers in the ...
Thanks to relatively firm mode identification, possible based on period ratios only, High Amplitude ...
We present the microlensing optical depth toward the Galactic bulge based on the detection of 99 eve...
The Chandra Galactic Bulge Survey (CGBS) is a shallow but wide survey of two approximately 6x1 degre...