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Related papers: Pulsating Variable Stars in the MACHO Bulge databa…

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We 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…

Based on a search for multi-periodic variability among the semi-regular red variable stars in the database of the All Sky Automated Survey (ASAS), a sample of 72 typical examples is presented. Their period analysis was performed using…

Solar and Stellar Astrophysics · Physics 2015-06-22 I. Fuentes-Morales , N. Vogt

We present the results of a systematic search for multiperiodic pulsators among the Galactic Bulge RR Lyrae stars of the OGLE-1 sample. We identify one "canonical" double-mode variable (RRd star) pulsating in two radial modes. In 38 stars…

Astrophysics · Physics 2009-11-07 P. Moskalik , E. Poretti

One hundred and forty six long-period red variable stars in the Large Magellanic Cloud (LMC) from the three year MOA project database were analysed. A careful periodic analysis was performed on these stars and a catalogue of their…

We study the brightness variations of galactic red supergiant stars using long-term visual light curves collected by the American Association of Variable Star Observers (AAVSO) over the last century. The full sample contains 48 red…

Astrophysics · Physics 2009-11-11 L. L. Kiss , Gy. M. Szabo , T. R. Bedding

Mid-infrared bright objects in the direction of the Galactic Bulge were investigated using time series photometry from the MACHO data archive, which led to the discovery of a large number of long-period variables. Among these, a total of…

Solar and Stellar Astrophysics · Physics 2016-12-05 Klaus Bernhard , Stefan Uttenthaler , Stefan Hümmerich

More than 1300 variables classified provisionally as first overtone RR Lyrae pulsators in the MACHO variable star database of the Large Magellanic Cloud (LMC) have been subjected to standard frequency analysis. Based on the remnant power in…

The first catalog of chromospherically active and ellipsoidal variable stars in the OGLE database is presented. The periods, the observed magnitudes and colors, their values free of interstellar extinction, and Fourier coefficients of light…

Astrophysics · Physics 2016-08-30 Arkadiusz Olech

We present the photometric properties of 1279 blue variable stars within the LMC. Photometry is derived from the MACHO database. The lightcurves of the sample exhibit a variety of quasi-periodic and aperiodic outburst behavior. A…

Astrophysics · Physics 2009-11-07 Stefan C. Keller , M. S. Bessell , K. H. Cook , M. Geha , D. Syphers

We have used long-term AAVSO visual observations and Fourier and wavelet analysis to identify periods and study long-term amplitude variations in 44 red supergiants. Of these, 12 stars had data which were too sparse and/or had low amplitude…

Solar and Stellar Astrophysics · Physics 2013-10-24 John R. Percy , Viraja C. Khatu

We obtained a series of more than two hundred R-band CCD images for the crowded central (115"x77") region of the metal-poor globular cluster M15 with an angular resolution of 0.5"-0.9" in most images. Optimal image subtraction was used to…

Astrophysics · Physics 2009-11-10 Alexander P. Zheleznyak , Valery V. Kravtsov

Several classes of pulsating stars are now known to undergo slow changes in amplitude; these include pulsating red giants and supergiants, and yellow supergiants. We have used visual observations from the AAVSO International Database, and…

Solar and Stellar Astrophysics · Physics 2014-05-30 John R. Percy , Jeong Yeon , Yook

It was recently discovered that the amplitudes of pulsating red giants and supergiants vary significantly on time scales of 20-30 pulsation periods. Here, we analyze the amplitude variability in 29 pulsating yellow supergiants (5 RVa, 4…

Solar and Stellar Astrophysics · Physics 2014-05-30 John R. Percy , Rufina Y. -H. Kim

Random changes in pulsation period are well established in cool pulsating stars, in particular the red giant variables: Miras, semi-regulars of types A and B, and RV Tau variables. Such effects are also observed in a handful of Cepheids,…

Solar and Stellar Astrophysics · Physics 2015-05-13 David G. Turner , J. R. Percy , T. Colivas , Leonid N. Berdnikov , Mohamed Abdel-Sabour Abdel-Latif

In this work, a sample of luminous M-type giants in the Baade's Windows towards the inner Galactic Bulge is investigated in the near-infrared. The ISOGAL survey at 7 and 15 micron has given information concerning the mass-loss rates of…

Astrophysics · Physics 2007-05-23 M. Schultheis , I. S. Glass

This paper reports on time-series analysis of 156 pulsating red giants (21 SRa, 52 SRb, 33 SR, 50 Lb) in the AAVSO (American Association of Variable Star Observers) observing program for which there are no more than 150-250 observations in…

Solar and Stellar Astrophysics · Physics 2018-04-24 John R. Percy

Red giants are unstable to radial pulsation. About a third of them also show a long secondary period, 5 to 10 times the pulsation period. The long secondary periods were recently ascribed to eclipses of the red giant by a low-mass…

Solar and Stellar Astrophysics · Physics 2022-09-20 John R. Percy

We discuss the results of a systematic search for multiperiodic pulsations in Galactic Bulge Delta Scuti and RR Lyrae stars. Six "normal" double-mode variables pulsating in two radial modes have been identified (5 Delta Scuti-type and 1 RR…

Astrophysics · Physics 2007-05-23 P. Moskalik , E. Poretti

We present the AGAPE astrometric and photometric catalogue of 1579 variable stars in a 14'x10' field centred on M31. This work is the first survey devoted to variable stars in the bulge of M31. The R magnitudes of the objects and the B-R…

This paper is the first part of the Catalog of Periodic Variable Stars in the Galactic bulge. The Catalog is based on observations collected during the OGLE microlensing search. 213 periodic variable stars brighter than I=18 mag: 31…

Astrophysics · Physics 2016-08-30 A. UDALSKI , M. KUBIAK , M. SZYMANSKI , J. KALUZNY , M. MATEO , W. KRZEMINSKI
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