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Related papers: Nonradial oscillations in classical Cepheids: the …

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The linear instability of thin, vertically-isothermal Keplerian discs, under the influence of axial magnetic field is investigated. Solutions of the stability problem are found explicitly by asymptotic expansions in the small aspect ratio…

Solar and Stellar Astrophysics · Physics 2015-06-03 E. Liverts , Yu. Shtemler , M. Mond

New results concerning the orbital stability of periodic traveling wave solutions for the "abcd" Boussinesq model will be shown in this manuscript. For the existence of solutions, we use basic tools of ordinary differential equations to…

Analysis of PDEs · Mathematics 2022-05-04 Gabriel E. Bittencourt Moraes , Guilherme de Loreno , Fábio Natali

In this paper, we discuss and examine various issues concerning the recent findings that suggested the observed period-luminosity (P-L) relation for the Large Magellanic Cloud (LMC) Cepheids is nonlinear. These include (1) visualizing the…

Astrophysics · Physics 2008-11-26 C. Ngeow , S. Kanbur

Only a fraction of the theoretically predicted nonradial pulsation modes have so far been observed in Delta Scuti stars. Nevertheless, the large number of frequencies detected in recent photometric studies of selected Delta Scuti stars…

Astrophysics · Physics 2015-05-13 M. Breger , P. Lenz , A. A. Pamyatnykh

Recent studies have revealed a hitherto unknown complexity of Cepheid pulsation. We implement local kernel regression to search for both period and amplitude modulations simultaneously in continuous time and to investigate their…

Solar and Stellar Astrophysics · Physics 2018-03-28 Maria Süveges , Richard Anderson

We present a grid on non-linear convective type-II Cepheid models. The dense model grids are computed for 0.6M_Sun and a range of metallicities ([Fe/H]=-2.0,-1.5,-1.0), and for 0.8M_Sun ([Fe/H]=-1.5). Two sets of convective parameters are…

Solar and Stellar Astrophysics · Physics 2016-01-18 R. Smolec

The present work investigates the numerical evolution of linearized oscillations of non-rotating, spherically symmetric neutron stars within the framework of general relativity. We derive the appropriate equations using the (3+1)-formalism.…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Johannes Ruoff

We consider stochastic perturbations of PDEs which have special pattern solutions, such as (nonlinear) travelling waves, solitons, and spiral waves. We show orbital stability of these patterns on a timescale which is exponential in the…

Dynamical Systems · Mathematics 2024-06-25 Joris van Winden

In this work we find explicit periodic wave solutions for the classical $\phi^4$-model, and study their corresponding orbital stability/instability in the energy space. In particular, for this model we find at least four different branches…

Analysis of PDEs · Mathematics 2020-05-22 José Manuel Palacios

We present new theoretical Period-Radius (PR) relations for first overtone Galactic Cepheids. Current predictions are based on several sequences of nonlinear, convective pulsation models at solar chemical composition (Y=0.28, Z=0.02) and…

Astrophysics · Physics 2009-11-06 G. Bono , W. P. Gieren , M. Marconi , P. Fouque'

We give a status report of convective Cepheid and RR Lyrae model pulsations. Some striking successes can be reported, despite the use of a rather simple treatment of turbulent convection with a 1D time-dependent diffusion equation for the…

Astrophysics · Physics 2015-06-24 J. Robert Buchler , Zoltan Kollath

The ratio of pulsation to radial velocity (the projection factor) is currently limiting the accuracy of the interferometric Baade-Wesselink method. This work aims at establishing a link between the line asymmetry evolution over the…

Astrophysics · Physics 2009-11-13 N. Nardetto , D. Mourard , P. Kervella , Ph. Mathias , A. Merand , D. Bersier

Period change studies give a window to probe into the evolution and dynamics of Cepheids. While evolutionary period changes have been well studied both observationally and theoretically, non-evolutionary period changes lack a systematic and…

Strange modes have been found in the radial spectrum of many luminous stars, most recently in Cepheids and RR Lyrae. We show that there is nothing strange about these modes -- they must exist even in the adiabatic limit. With a change of…

Astrophysics · Physics 2008-02-03 J. R. Buchler , P. A. Yecko , Z. Kollath

We present new high-resolution (R=40000) spectroscopic observations of 18 bright northern Cepheids carried out at David Dunlap Observatory, in 1997. The measurements mainly extend those of presented in Paper I adding three more stars (AW…

Astrophysics · Physics 2009-10-31 L. L. Kiss , J. Vinko

The discovery of $\beta$ Cephei stars in low metallicity environments, as well as the difficulty in theoretically explaining the excitation of the pulsation modes observed in some $\beta$ Cephei and hybrid SPB-$\beta$ Cephei pulsators,…

Astrophysics · Physics 2008-11-26 A. Miglio , J. Montalban , M. -A. Dupret

A selection of known and newly-discovered northern hemisphere Cepheids and related objects are being monitored regularly through CCD observations at the automated Abbey Ridge Observatory, near Halifax, and photoelectric photometry from the…

Solar and Stellar Astrophysics · Physics 2015-05-13 David G. Turner , Daniel J. Majaess , David J. Lane , L. Szabados , V. V. Kovtyukh , I. A. Usenko , Leonid N. Berdnikov

We present the first part of a new catalog of variable stars (OIII-CVS) compiled from the data collected in the course of the third phase of the Optical Gravitational Lensing Experiment (OGLE-III). In this paper we describe the catalog of…

The effect of metallicity on the theoretical and empirical period-luminosity (PL) relations of Cepheid variables is not well understood and remains a highly debated issue. Here, we examine empirical colour-magnitude diagrams (CMDs) of…

Solar and Stellar Astrophysics · Physics 2024-04-29 Mami Deka , Earl P. Bellinger , Shashi M. Kanbur , Sukanta Deb , Anupam Bhardwaj , Hugh Riley Randall , Selim Kalici , Susmita Das

[Abridged] We aim to improve the understanding of Cepheids from an evolutionary perspective and establish the role of rotation in the Cepheid paradigm. In particular, we are interested in the contribution of rotation to the problem of…

Solar and Stellar Astrophysics · Physics 2014-06-11 R. I. Anderson , S. Ekström , C. Georgy , G. Meynet , N. Mowlavi , L. Eyer
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