The MACHO variables of LMC field 77 that lie in the vicinity of the Cepheid instability strip are reexamined. Among the 144 variables that we identify as Cepheids, we find 14 that have Fourier amplitudes <0.05 mag in the MACHO red band, of which seven have an amplitude <0.006 mag: we dub the latter group of stars ultralow-amplitude (ULA) Cepheids. The variability of these objects is verified by a comparison of the MACHO red with the MACHO blue light curves and with those of the corresponding OGLE LMC stars. The occurrence of ULA Cepheids is in agreement with theory. We have also discovered two low-amplitude variables whose periods are about a factor of 5-6 smaller than those of F Cepheids of equal apparent magnitude. We suggest that these o...
Cepheids are sensitive astrophysical laboratories that probe internal mixing processes and convectio...
We have frequency-analyzed 6391 variables classified earlier as fundamental-mode RR Lyrae (RRO) star...
We present the results of nonlinear pulsation modeling of 20 bump Cepheids in the LMC. By obtaining ...
A search for variable stars with ultra-low amplitudes (ULAs), in the millimagnitude range, has been ...
We present an analysis of the period distribution of about 1800 Cepheids in the LMC, based on data o...
Context. The properties of variable stars can give independent constraints on the star formation hi...
This is a progress report of the study of pulsating main-sequence stars in the LMC. Using the OGLE-I...
We present a method for solving the light curve of an eclipsing binary system that contains a Cephei...
A thorough analysis of the OGLE-II time-series photometry of the Large Magellanic Cloud bar suppleme...
We report the of the existence of RV Tauri stars in the Large Magellanic Cloud (LMC). This class of ...
We present a method for solving the light curve of an eclipsing binary system that contains a Cephei...
We present CCD phase-binned light curves at 490\,nm for 97 Cepheid variable stars in the bar of the ...
We present a period-luminosity-amplitude analysis of 5899 red giant and binary stars in the Large Ma...
Cepheids are important distance indicators in the local Universe and key objects for testing the pre...
We have frequency analyzed 6391 variables classified earlier as fundamental mode RR Lyrae (RR0) star...
Cepheids are sensitive astrophysical laboratories that probe internal mixing processes and convectio...
We have frequency-analyzed 6391 variables classified earlier as fundamental-mode RR Lyrae (RRO) star...
We present the results of nonlinear pulsation modeling of 20 bump Cepheids in the LMC. By obtaining ...
A search for variable stars with ultra-low amplitudes (ULAs), in the millimagnitude range, has been ...
We present an analysis of the period distribution of about 1800 Cepheids in the LMC, based on data o...
Context. The properties of variable stars can give independent constraints on the star formation hi...
This is a progress report of the study of pulsating main-sequence stars in the LMC. Using the OGLE-I...
We present a method for solving the light curve of an eclipsing binary system that contains a Cephei...
A thorough analysis of the OGLE-II time-series photometry of the Large Magellanic Cloud bar suppleme...
We report the of the existence of RV Tauri stars in the Large Magellanic Cloud (LMC). This class of ...
We present a method for solving the light curve of an eclipsing binary system that contains a Cephei...
We present CCD phase-binned light curves at 490\,nm for 97 Cepheid variable stars in the bar of the ...
We present a period-luminosity-amplitude analysis of 5899 red giant and binary stars in the Large Ma...
Cepheids are important distance indicators in the local Universe and key objects for testing the pre...
We have frequency analyzed 6391 variables classified earlier as fundamental mode RR Lyrae (RR0) star...
Cepheids are sensitive astrophysical laboratories that probe internal mixing processes and convectio...
We have frequency-analyzed 6391 variables classified earlier as fundamental-mode RR Lyrae (RRO) star...
We present the results of nonlinear pulsation modeling of 20 bump Cepheids in the LMC. By obtaining ...