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相关论文: Metallicity Effects on RR Lyrae Variables

200 篇论文

We found a possible relationship between the modulation period and the amplitude of the Blazhko RR Lyrae stars: long modulation period generally implies high modulation amplitude while the short modulation period results in small amplitude.…

太阳与恒星天体物理 · 物理学 2015-10-21 J. M. Benkő , R. Szabó

We discuss results of an exploratory non-LTE analysis of two metal-rich A-type supergiants in M31. Using comprehensive model atoms we derive accurate atmospheric parameters from multiple indicators and show that non-LTE effects on the…

天体物理学 · 物理学 2007-05-23 Norbert Przybilla , Keith Butler , Rolf-Peter Kudritzki

A high percentage of the astrophysically important RR Lyrae stars show a periodic amplitude and/or phase modulation of their pulsation cycles. More than a century after its discovery, this "Blazhko effect" still lacks acceptable theoretical…

太阳与恒星天体物理 · 物理学 2009-10-02 Katrien Kolenberg , Stefano Bagnulo

Additional low-amplitude signals are observed in many RR Lyrae stars, beside the pulsations in radial modes. The most common ones are short-period signals forming a period ratio of around 0.60--0.65 with the first overtone, or long-period…

太阳与恒星天体物理 · 物理学 2023-09-27 H. Netzel , L. Molnar , E. Plachy , J. M. Benko

Rigorous electrodynamical simulations based on the nonlinear Drude model are performed to investigate the influence of strong coupling on high harmonic generation by periodic metal gratings. It is shown that a thin dispersive material with…

介观与纳米尺度物理 · 物理学 2019-08-13 Elena Drobnyh , Ruth Pachter , Maxim Sukharev

Recent dramatic improvements in the modeling of abundance evolution due to diffusion in A stars have been achieved with the help of monochromatic opacity tables from the OPAL group. An important result in the context of stellar pulsations…

天体物理学 · 物理学 2007-05-23 S. Turcotte , J. Richer , G. Michaud , J. Christensen-Dalsgaard

We present B and V CCD photometry for variables in the cluster central region, adding new data for 32 variables and giving suitable light curves, mean magnitudes and corrected colors for 17 RR Lyrae. Implementing the data given in this…

天体物理学 · 物理学 2009-10-31 F. Caputo , V. Castellani , M. Marconi , V. Ripepi

We provide theoretical and numerical tools to quantitatively study the impact of nonlocality arising from free electrons in metals on the optical properties of metallo-dielectric multilayers. Though effects due to nonlocality are in general…

Compilations of abundances of Strontium and Barium in extremely metal-poor stars show that an apparent cutoff is observed for [Sr/Ba] at [Fe/H]$<$-3.6 and large fluctuations for [Fe/H]$>$-3.6 with a clear upper bound depending on…

太阳与恒星天体物理 · 物理学 2015-06-15 Wako Aoki , Takuma Suda , Richard Boyd , Toshitaka Kajino , Michael Famiano

The fluorescence of organic fluorophore molecules is enhanced when they are placed in contact with certain metals (Al, Ag, Cu, Au, etc.) whose surface plasmon waves couple into the radiative modes of the molecules and increase the radiative…

介观与纳米尺度物理 · 物理学 2015-04-21 S. Sarkar , B. Kanchibotla , J. D. Nelson , J. D. Edwards , J. Anderson , G. C. Tepper , S. Bandyopadhyay

Evolutionary models have been calculated for Pop II stars of 0.5 to 1.0$M_\odot$ from the pre-main-sequence to the lower part of the giant branch. Rosseland opacities and radiative accelerations were calculated taking into account the…

天体物理学 · 物理学 2008-11-26 O. Richard , G. Michaud , J. Richer , S. Turcotte , S. Turck-Chieze , Don A. VandenBerg

We examine the role of opacities in stellar pulsation with reference to Cepheids and RR Lyraes, and examine the effect of augmented opacities on the theoretical pulsation light curves in key temperature ranges. The temperature ranges are…

太阳与恒星天体物理 · 物理学 2018-06-11 S. M. Kanbur , M. Marconi , A. Bhardwaj , R. Kundu , H. P. Singh

We present infrared observations of 66 starburst galaxies over a wide range of oxygen abundances, to measure how metallicity affects their dust properties. The data include imaging and spectroscopy from the Spitzer Space Telescope,…

We report the discovery of a new subclass of double-mode RR Lyrae stars in the Large and Small Magellanic Clouds. The sample of 22 pulsating stars have been extracted from the latest edition of the OGLE collection of RR Lyrae variables in…

We present a detailed abundance analysis of high-resolution ultraviolet echelle spectra of five subdwarf B stars obtained with HST-STIS The goal of our observations was to test the hypothesis that pulsations in sdBs are correlated to the…

天体物理学 · 物理学 2007-05-23 S. O'Toole , U. Heber

By using a large sample of published spectroscopic iron abundances, we point out the importance of gravity correction in deriving more accurate metal abundances for RR Lyrae stars. For the 197 stars with multiple spectra we find overall…

太阳与恒星天体物理 · 物理学 2023-10-18 Geza Kovacs , Johanna Jurcsik

The surface gravities and effective temperatures have been added to a compilative catalog published earlier, which includes the relative abundances of several chemical elements for 100 field RR Lyrae stars. These atmoshperic parameters and…

星系天体物理 · 物理学 2019-03-29 V. A. Marsakov , M. L. Gozha , V. V. Koval'

A new, extended time-series photometry of M3 RR Lyrae stars has revealed that four of the ten double-mode stars show large-amplitude Blazhko modulation of both radial modes. The first, detailed analysis of the peculiar behavior of the…

太阳与恒星天体物理 · 物理学 2015-06-23 J. Jurcsik , P. Smitola , G. Hajdu , J. Nuspl

delta Scuti variables are stars which exhibit periodic changes in their luminosity through radial and non-radial pulsations. Internally, these stars have relatively small convective cores, and convective overshoot can significantly affect…

太阳与恒星天体物理 · 物理学 2022-01-26 V. Dornan , C. C. Lovekin

We discuss two topics on the experimental measurements of fluctuation observables in relativistic heavy-ion collisions. First, we discuss the effects of the thermal blurring, i.e. the blurring effect arising from the experimental…

核理论 · 物理学 2016-10-21 Masakiyo Kitazawa , Masayuki Asakawa