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We carry out an extensive light curve comparison of BL Her stars using observations from Gaia DR3 and stellar pulsation models computed using MESA-RSP with the goal to obtain the best-matched modeled-observed pairs for BL Her stars in the…

We present the most extensive set to date of high-quality RR Lyrae light curve templates in the griz bands, based on time-series observations of the Dark Energy Camera Plane Survey (DECaPS) East field, located in the Galactic bulge at…

We present a sample of ~5,000 RR Lyrae stars selected from the recalibrated LINEAR dataset and detected at heliocentric distances between 5 kpc and 30 kpc over ~8,000 deg^2 of sky. The coordinates and light curve properties, such as period…

We present a careful and detailed light curve analysis of publicly available $I$-band data on fundamental mode RR Lyrae (RRab) stars of the Large Magellanic Cloud (LMC) obtained by the Optical Gravitational Lensing Experiment (OGLE)…

太阳与恒星天体物理 · 物理学 2015-06-18 Sukanta Deb , Harinder P. Singh

One of the major science goals of the SkyMapper Survey of the Southern Hemisphere sky is the determination of the shape and extent of the halo of the Galaxy. In this paper we quantify the likely efficiency and completeness of the survey as…

太阳与恒星天体物理 · 物理学 2015-06-17 S. Akhter , G. S. Da Costa , S. C. Keller , B. P. Schmidt , M. S. Bessell , P. Tisserand

We present the results of a deep, wide-area variability survey in the Southern hemisphere, the first of its kind. As part of the Catalina Sky Surveys, the Siding Spring Survey (SSS) has covered $14,800$ square degrees in the declination…

We have applied the image subtraction method to the M3 dataset previously analyzed by Corwin & Carney (2001; CC01). The new analysis produced light curves and periods for 15 variables, bringing to 222 the total number of RR Lyrae stars in…

天体物理学 · 物理学 2009-11-10 G. Clementini , T. M. Corwin , B. W. Carney , A. N. Sumerel

We present a multiband (UBVRI) time-series photometric study of RR Lyrae (RRL) stars in the globular cluster Messier 53 (NGC 5024) to refine their pulsation properties and determine a precise cluster distance. The archival photometric data…

太阳与恒星天体物理 · 物理学 2026-01-08 Shantanu A. Gaur , Nitesh Kumar , Anupam Bhardwaj , Aasheesh Raturi

In this paper we present new CCD investigations of RR Lyrae pulsators in the Oo.I globular cluster M5. B V curves of light for 15 RR Lyrae are presented. With the addition of further 11 curves of light by Storm, Carney and Beck (1991) one…

天体物理学 · 物理学 2009-10-28 E. Brocato , V. Castellani , V. Ripepi

In this paper we report the discovery of 35 new RR Lyrae variables. These stars were found by a special searching technique. We crossmatched the catalog of the PanSTARRS (PS) sky survey with K2 space photometry data to the validate…

太阳与恒星天体物理 · 物理学 2018-03-28 Áron L. Juhász , László Molnár

The properties of RR Lyrae variables make them excellent probes of the formation and evolution of a stellar population. The mere presence of such stars necessitates an age greater than ~10 Gyr while their periods and amplitudes can be used…

星系天体物理 · 物理学 2011-05-26 Ata Sarajedini

Str\"omgren uvby-beta photometry is reported for the RR Lyrae stars AE, RS, ST, TV, TW, UU, and XX in Bootes. The physical parameters M/Mo, log (L/Lo), M_V, log T_eff and [Fe/H], have been estimated from the Fourier decomposition of the…

太阳与恒星天体物理 · 物理学 2009-07-28 J. H. Peña , A. Arellano Ferro , R. Peña Miller , J. P. Sareyan , M. Alvarez

Measurements of [Fe/H] and radial velocity are presented for 89 RR Lyrae (RRL) candidates within 6 kpc of the Sun. After removal of two suspected non-RRL, these stars were added to an existing database, which yielded 464 RRL with [Fe/H] on…

星系天体物理 · 物理学 2020-01-08 R. Zinn , X. Chen , A. C. Layden , D. I. Casetti-Dinescu

We have measured the periods and light curves of 148 RR Lyrae variables from V=13.5 to 19.7 from the first 100 sq. degrees of the QUEST RR Lyrae survey. Approximately 55% of these stars belong to the clump of stars detected earlier by the…

New BVI CCD photometry is presented for 60 RR Lyrae variables in the globular cluster M3. Light curves have been constructed and ephemerides have been (re)-derived for all of them. Four stars (i.e. V29, V136, V155 and V209), although…

天体物理学 · 物理学 2009-10-30 E. Carretta , C. Cacciari , F. R. Ferraro , F. Fusi Pecci , G. Tessicini

We present a calibration of the metallicity and physical parameters (temperature, luminosity, gravity, mass, radius) for RR Lyrae stars using the ugriz SDSS photometric system. Our work is based on calculations of synthetic horizontal…

太阳与恒星天体物理 · 物理学 2015-06-12 M. Catelan , G. I. Torrealba , C. Caceres , H. A. Smith , N. De Lee , M. Fitzgerald

We compiled a list of about 250 SX Phoenicis stars known in Galactic globular clusters in order to study period-luminosity relation for this type of variable. The absolute magnitudes of these stars are derived using metallicity-luminosity…

太阳与恒星天体物理 · 物理学 2012-11-26 Grzegorz Kopacki , Andrzej Pigulski

Discoveries of RR Lyrae and Cepheid variable stars with multiple modes of pulsation have increased tremendously in recent years. The Fourier spectra of these stars can be quite complicated due to the large number of combination frequencies…

太阳与恒星天体物理 · 物理学 2016-07-07 Earl P. Bellinger , Daniel Wysocki , Shashi M. Kanbur

(Abridged) We present CCD BVI photometry of 85 variable stars from the field of the globular cluster NGC 6934. The photometry was obtained with the image subtraction package ISIS. 35 variables are new identifications: 24 RRab stars, 5 RRc…

天体物理学 · 物理学 2009-10-31 J. Kaluzny , A. Olech , K. Z. Stanek

With the aid of the All Sky Automated Survey (ASAS) database on the Galactic field, we compare the iron abundances of fundamental mode RR Lyrae stars derived from the Fourier parameters with those obtained from low-dispersion spectroscopy.…

天体物理学 · 物理学 2009-11-11 Geza Kovacs