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Relevant bibliographies by topics / Stellar oscillations. Variable stars

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Dissertations / Theses
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Academic literature on the topic 'Stellar oscillations. Variable stars'

Author: Grafiati

Published: 4 June 2021

Last updated: 11 February 2022

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Journal articles on the topic "Stellar oscillations. Variable stars"

1

Giménez, Alvaro, Steven D. Kawaler, Conny Aerts, et al. "DIVISION V: VARIABLE STARS." Proceedings of the International Astronomical Union 4, T27A (2008): 251–53. http://dx.doi.org/10.1017/s1743921308025623.

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Division V deals with all aspects of stellar variability, either intrinsic or due to eclipses by its companion in a binary system. In the case of intrinsic stellar variability the analysis of pulsating stars, surface inhomogeneities, stellar activity and oscillations are considered. For close binaries, classical detached eclipsing binaries are studied as well as more interacting systems, like contact and semi-detached binaries, or those with compact components, like cataclysmic variables and X-ray binaries, including the physics of accretion processes.

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Chitre, S. M. "Excitation and damping of solar and stellar oscillations." Symposium - International Astronomical Union 123 (1988): 345–57. http://dx.doi.org/10.1017/s0074180900158346.

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Variable stars can be broadly classified into two categories: (a) High amplitude pulsators like Cepheids and RR Lyrae variables, (b) Low amplitude pulsators like Sun and Sun-like stars. The study of stellar pulsations has opened the possibility of using the oscillatory modes to probe the internal structure and dynamics of these stars. The cause of pulsational instability for a majority of stars is the partial ionisation of the abundant elements present in the envelope of the stars, while some instabilities are driven by the transfer of momentum from the medium to the oscillating elements. Vari

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Waelkens, C. "Pulsation and Evolution. An observer’s viewpoint." International Astronomical Union Colloquium 155 (1995): 23–30. http://dx.doi.org/10.1017/s0252921100036733.

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AbstractWe review observational evidence on the interaction between stellar pulsation and evolution. We discuss to what extent observations of pulsating stars with variable amplitudes and pulsation periods have implications on our understanding of stellar structure and evolution. The probable link between mass loss and pulsation in AGB stars and in hot luminous stars appears to be the strongest way in which pulsations affect evolution. We point out the possibility that forced oscillations in the components of binaries may have important consequences on evolution, that could offer an explanatio

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Ahlers, John P., Jason W. Barnes, Sarah A. Horvath, Samuel A. Myers, and Matthew M. Hedman. "LASR-guided stellar photometric variability subtraction." Astronomy & Astrophysics 615 (July 2018): A128. http://dx.doi.org/10.1051/0004-6361/201732446.

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We develop a technique for removing stellar variability in the light curves of δ-Scuti and similar stars. Our technique, which we name the Linear Algorithm for Significance Reduction (LASR), subtracts oscillations from a time series by minimizing their statistical significance in frequency space. We demonstrate that LASR can subtract variable signals of near-arbitrary complexity and can robustly handle close frequency pairs and overtone frequencies. We demonstrate that our algorithm performs an equivalent fit as prewhitening to the straightforward variable signal of KIC 9700322. We also show t

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Warner, Brian, and Patrick A. Woudt. "Quasi-Periodic Oscillations in Accretion Discs." International Astronomical Union Colloquium 185 (2002): 584–85. http://dx.doi.org/10.1017/s0252921100017164.

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Quasi-Periodic Oscillations (QPOs) in Cataclysmic Variable stars (CVs) with periods in the range 100 – 2000 s have been known for 25 years (see Chapter 8 of Warner, 1995a). We distinguish here between QPOs and Dwarf Nova Oscillations (DNOs) – the latter being of shorter period (5 – 50 s) and greater coherence. QPOs appear as brightness modulations and typically have quite short coherence lengths (a few cycles).QPOs are largely associated with discs transferring mass at a high rate – i.e., dwarf novae during outburst or nova-like variables; but the QPOs are not always present and many systems h

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Däppen, W., W. A. Dziembowski, and R. Sienkiewicz. "Asteroseismology: results and prospects." Symposium - International Astronomical Union 123 (1988): 233–47. http://dx.doi.org/10.1017/s0074180900158140.

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Asteroseismology is interpreted as an extension of the field of variable stars, and not just as the stellar analogue of helioseismology. The main effects of stellar mass and evolution on oscillation frequencies are discussed with the help of simplified wave-propagation diagrams. Frequency separations resulting from asymptotic expressions are compared with the corresponding results from numerical computations. The validity of asymptotic theory can be gauged in this way. The seismological issues of solar-like stars and Ap stars are discussed in some detail, and a progress report on the equation

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Moffat, Anthony F. J. "Asteroseismology of massive stars with the MOST satellite." Proceedings of the International Astronomical Union 5, H15 (2009): 366. http://dx.doi.org/10.1017/s174392131000983x.

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AbstractSince 2003 the MOST (Microvariability and Oscillations of STars) microsatellite has obtained typically a month of non-stop, minute-of-time resolution, high-precision, single-broadband optical photometry for each of a significant number of Galactic OB and WR stars. Numerous p- and g-modes were clearly detected in several OB stars, including discovery of g-modes for the first time in a blue supergiant (Saio et al. 2006). True rotation periods were found for some SPBe pulsators (Cameron et al. 2008). Many O stars are remarkably quiet. Five presumably single WR stars have been observed so

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8

Rodríguez, E., L. A. Balona, M. J. López-González, S. Ocando, S. Martín-Ruiz, and C. Rodríguez-López. "Pulsation and rotation in NGC 6811: the Kepler short-cadence stars." Monthly Notices of the Royal Astronomical Society 491, no. 3 (2019): 4345–64. http://dx.doi.org/10.1093/mnras/stz3143.

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ABSTRACT We have analysed a selected sample of 36 Kepler short-cadence stars in the field of NGC 6811. The results reveal that all the targets are variable: two red giant stars with solar-like oscillations, 21 main-sequence pulsators (16 δ Scuti and five γ Doradus stars), and 13 rotating variables. Three new γ Doradus (γ Dor) variables (one is a hot γ Dor star) are detected in this work together with five new rotating variables. An in-depth frequency analysis of the δ Scuti (δ Sct) and γ Dor stars in the sample shows that the frequency spectra are very rich, in particular for the δ Sct-type va

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Haucke, M., L. S. Cidale, R. O. J. Venero, et al. "Wind properties of variable B supergiants." Astronomy & Astrophysics 614 (June 2018): A91. http://dx.doi.org/10.1051/0004-6361/201731678.

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Context. Variable B supergiants (BSGs) constitute a heterogeneous group of stars with complex photometric and spectroscopic behaviours. They exhibit mass-loss variations and experience different types of oscillation modes, and there is growing evidence that variable stellar winds and photospheric pulsations are closely related. Aims. To discuss the wind properties and variability of evolved B-type stars, we derive new stellar and wind parameters for a sample of 19 Galactic BSGs by fitting theoretical line profiles of H, He, and Si to the observed ones and compare them with previous determinati

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Dziembowski, W. A. "Mode Selection and Other Nonlinear Phenomena in Stellar Oscillations." International Astronomical Union Colloquium 137 (1993): 521–34. http://dx.doi.org/10.1017/s0252921100018352.

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AbstractNonlinear effects determining the amplitudes of unstable modes of oscillations in stellar modes, are reviewed. The two basic processes - saturation of the driving mechanism and resonant mode coupling - are discussed within the framework of the amplitude equation formalism. There are difficult problems in the theory of multiple mode interaction that must be solved to make a prediction of amplitude spectra possible. The observed spectra for δ Scu stars and other multiperiodic variables, exhibit no simple pattern that would suggest a solution of the theoretical problems.

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Dissertations / Theses on the topic "Stellar oscillations. Variable stars"

1

Matalgah, Ziyad. "Second Order Rotational Effect On Nonradial Oscillations In Delta-scuti Stars." Master's thesis, METU, 2004. http://etd.lib.metu.edu.tr/upload/12604741/index.pdf.

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In this work the effect of rotation on oscillation frequencies have been inves- tigated . Rotation has been treated as a perturbation and detailed calculations were done on the infuence of second order rotation . We used an evolutionary model of DELTA-Scuti star V1162 Ori with a mass of 1:8 solar mass. The eigenfrequencies were calculated in two cases , the slow rotation case with vsini = 46km/s and the fast rotation case with vsini = 61.9km/s. Calculation were carried out by a modifed oscillation program and results were compared to observations .

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Pretorius, Magaretha L. "Rapid oscillations in cataclysmic variable stars." Master's thesis, University of Cape Town, 2004. http://hdl.handle.net/11427/6103.

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Includes bibliographical references (p. 129-146).<br>Rapid quasi-coherent oscillations were detected in the optical light curves of 24 cataclysmic variable stars (CVS). In 12 of these systems (TU Men, WW Cet, HX Peg, BP CrA, BR Lup, HP Nor, AG Hya, TW Vir, PU CMa, V426 Ooph, V1193 Ori, and CR Boo) for the first time. The results contribute to the observational record of the phenomenology of dwarf nova oscillations (DNOs), quasi-periodic oscillations (QPOs), and longer period dwarf nova oscillations (lpDNOs), strengthen the correlation, valid over nearly six orders of magnitude in frequency, be

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Kennelly, Edward James. "Nonradial pulsations of rapidly rotating [delta] Scuti stars." Thesis, University of British Columbia, 1990. http://hdl.handle.net/2429/29140.

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Time series of high resolution CFHT spectra of four δ Scuti stars are examined for consistency with the presence of nonradial pulsations (nrp). Each series exhibits a progression of subfeatures moving from blue to red through the absorption lines. We have reproduced the profile variations using a geometrical model which imposes sectorial modes on the surface of the star. Modeling of the low-degree modes is guided by radial-velocity variations and the known photometric variations. Synthetic spectra generated with the appropriate Teff and log g for each star are used as input for the model. In

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Weldrake, David Thomas Frederick. "Giant planets and variable stars in globular clusters /." View thesis entry in Australian Digital Theses Program, 2005. http://thesis.anu.edu.au/public/adt-ANU20050616.191315/index.html.

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Davey, Stephen. "Irradiation of the secondary star in cataclysmic variable stars." Thesis, University of Sussex, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.386388.

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Munteanu, Andreea. "Nonlinear one-zone models of stellar pulsations." Doctoral thesis, Universitat Politècnica de Catalunya, 2003. http://hdl.handle.net/10803/6610.

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Nuestro trabajo se ha concentrado en la simulación y el análisis de modelos no-lineales aplicados a las curvas de luz ópticas de estrellas variables de largo periodo. Cuando las estrellas de masa pequeña o intermedia (de 1 a 11 masas solares) llegan a las fases finales de su evolución, tales como la Rama Asintótica de las (Super-)Gigantes, presentan oscilaciones regulares e irregulares de larga duración (i.e. estrellas Miras). Las pulsaciones regulares e irregulares facilitan los episodios de pérdida de masa y hacen que estas estrellas jueguen un papel crucial en la evolución química de la

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Drake, A. J., S. G. Djorgovski, M. Catelan, et al. "The Catalina Surveys Southern periodic variable star catalogue." OXFORD UNIV PRESS, 2017. http://hdl.handle.net/10150/625504.

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Here, we present the results from our analysis of 6 yr of optical photometry taken by the Siding Spring Survey (SSS). This completes a search for periodic variable stars within the 30 000 deg(2) of the sky covered by the Catalina Surveys. The current analysis covers 81 million sources with declinations between -20 degrees. and -75 degrees. with median magnitudes in the range 11 < V < 19.5. We find approximately 34 000 new periodic variable stars in addition to the similar to 9000 RR Lyrae that we previously discovered in SSS data. This brings the total number of periodic variables identified i

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Agüeros, Marcel A. "Candidate isolated neutron stars and other stellar x-ray sources from the ROSAT all-sky and Sloan Digital Sky Surveys /." Thesis, Connect to this title online; UW restricted, 2006. http://hdl.handle.net/1773/5436.

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Dogan, Gulnur. "The Effect Of Rotation, Up To Second Order, On The Oscillation Frequencies Of Some Delta-scuti Stars." Master's thesis, METU, 2007. http://etd.lib.metu.edu.tr/upload/12608873/index.pdf.

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In this work, the effect of rotation on the oscillation frequencies of some radially and nonradially oscillating Delta-Scuti stars have been explored. Rotation has been considered as a perturbation and treated up to the second order. Series of evolutionary models have been calculated for the oscillating stars in question and compared with the observational parameters. Three stars are considered: V350 Peg with no rotation, CC And with a rotational velocity Vsini=20 km/s, and BS Tuc with Vsini=130 km/s. We find that splitting in the oscillation frequencies are conspicuous especially in fast rota

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Plaks, Irina. "Mapping the Early Galaxy: RR Lyrae Kinematics and Metallicities." Bowling Green State University / OhioLINK, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=bgsu1627059931940409.

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Books on the topic "Stellar oscillations. Variable stars"

1

1953-, Nemec James Michael, and Matthews Jaymie M, eds. New perspectives on stellar pulsation and pulsating variable stars: Proceedings of IAU Colloquium no. 139, Victoria, British Columbia, 15-18, July 1992. Cambridge University Press, 1993.

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2

M, Pap Judit, ed. The sun as a variable star: Solar and stellar irradiance variations : proceedings of IAU Colloquium no. 143, held in Boulder, Colorado, USA, June 20-25, 1993. Cambridge University Press, 1994.

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Colloquium, International Astronomical Union. The sun as a variable star: Solar and stellar irradiance variations : proceedings of the 143rd Colloquium of the International Astronomical Union held in the Clarion Harvest House, Boulder, Colorado, June 20-25, 1993. Kluwer Academic Publishers, 1994.

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1914-, Ledoux Paul, Smeyers Paul, Aerts Conny, Bedding T. R, and Christensen-Dalsgaard Jørgen 1950-, eds. Radial and nonradial pulsations as probes of stellar physics: IAU Colloquium 185 : proceedings of a colloquium held at Institute of Astronomy, Catholic University of Leuven, Leuven, Belgium, 26-31 July, 2001. Astronomical Society of the Pacific, 2002.

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Wolf, Bernhard, Otmar Stahl, and Alex W. Fullerton, eds. Variable and Non-spherical Stellar Winds in Luminous Hot Stars. Springer Berlin Heidelberg, 1999. http://dx.doi.org/10.1007/bfb0106346.

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Johnson, Hollis R. The M-type stars. Centre national de la recherche scientifique ; NASA Scientific and Technical Information Branch, 1986.

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Rozelot, J. P. The Pulsations of the Sun and the Stars. Springer-Verlag Berlin Heidelberg, 2011.

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IAU, Colloquium (155th 1995 Cape Town South Africa). Astrophysical applications of stellar pulsation: Proceedings of IAU colloquium 155, held in Cape Town, 6-10 February 1995. Astronomical Society of the Pacific, 1995.

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9

Shibahashi, H., and Anthony Eugene Lynas-Gray. Progress in physics of the sun and stars: A new era in helio- and asteroseismology : proceedings of a Fujihara Seminar held at Hakone, Japan, in 25-29 November 2012. Astronomical Society of the Pacfic, 2013.

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Torben, Arentoft, Gonzaléz Hernández Irene, Lindsey, Charles (Charles Allan), 1947-, Hill Frank 1952-, Global Oscillations Network Group. GONG 2008, and SOHO Workshop (21st : 2008 : Boulder, Co.), eds. Solar-stellar dynamos as revealed by helio- and asteroseismology: GONG 2008 / SOHO 21 ; Proceedings of a conference held at the High Altitude Observatory, Boulder, Colorado, USA, 11-15 August 2008. Astronomical Society of the Pacific, 2009.

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Book chapters on the topic "Stellar oscillations. Variable stars"

1

Audard, N., and J. Provost. "On P-Mode Oscillations in Stars from 1 M⊙ to 2 M⊙." In The Sun as a Variable Star: Solar and Stellar Irradiance Variations. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0950-5_50.

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2

Staude, J., N. S. Dzhalilov, and Y. D. Zhugzhda. "Radiation-Hydrodynamic Waves and Global Solar Oscillations." In The Sun as a Variable Star: Solar and Stellar Irradiance Variations. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0950-5_35.

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Paternò, L., and S. Sofia. "EUDOSSO: A Space Project for Solar Oscillations and Long Term Variability Relevant to Climatic Changes." In The Sun as a Variable Star: Solar and Stellar Irradiance Variations. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0950-5_45.

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Yip, C. W., M. C. Chu, and P. T. Leung. "Oscillations of Quark Stars." In Stellar Astrophysics. Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-010-0878-5_19.

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Hoffmeister, Cuno, Gerold Richter, and Wolfgang Wenzel. "The Significance of Variable Stars for Research on the Structure of the Galaxy and Stellar Evolution." In Variable Stars. Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/978-3-642-82269-8_7.

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Lee, Umin. "Low-Frequency Oscillations in Rotating Stars." In Studying Stellar Rotation and Convection. Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-33380-4_7.

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Xiong, D. R., Q. L. Cheng, and L. Deng. "Oscillations of HB Red Variable Stars." In New Eyes to See Inside the Sun and Stars. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4982-2_91.

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Rood, Robert T. "Non-Variable Horizontal-Branch Stars." In Fundamental Stellar Properties: The Interaction Between Observation and Theory. Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5602-8_48.

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Perdang, J. "Asymptotics and Quantum Chaos in Stellar Oscillations." In Seismology of the Sun and the Distant Stars. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4608-8_15.

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Christensen-Dalsgaard, Jørgen, and Woiciech A. Dziembowski. "Basic Aspects of Stellar Structure and Pulsation." In Variable Stars as Essential Astrophysical Tools. Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-011-4299-1_1.

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Conference papers on the topic "Stellar oscillations. Variable stars"

1

Varadi, Mihaly, Laurent Eyer, Stefan Jordan, et al. "Detecting Short Period Variable Stars with Gaia." In STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION: Proceedings of the International Conference. AIP, 2009. http://dx.doi.org/10.1063/1.3246507.

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Kaaret, Philip. "Spectral signatures of kilohertz quasiperiodic oscillations from accreting neutron stars." In X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. AIP, 2001. http://dx.doi.org/10.1063/1.1434631.

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Greco, Claudia, Nami Mowlavi, Laurent Eyer, et al. "Searching for Variable Stars in Galactic Open Clusters." In STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION: Proceedings of the International Conference. AIP, 2009. http://dx.doi.org/10.1063/1.3246502.

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Soszyński, Igor, Joyce Ann Guzik, and Paul A. Bradley. "The OGLE-III Catalog of Variable Stars 100 k Pulsating Stars in the LMC." In STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION: Proceedings of the International Conference. AIP, 2009. http://dx.doi.org/10.1063/1.3246499.

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Strohmayer, Tod E. "Oscillations during thermonuclear X-ray bursts: A new probe of neutron stars." In X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. AIP, 2001. http://dx.doi.org/10.1063/1.1434650.

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Jeon, Young-Beom, James M. Nemec, Alistair R. Walker, Joyce Ann Guzik, and Paul A. Bradley. "Variable Stars in the LMC Globular Cluster NGC 2210." In STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION: Proceedings of the International Conference. AIP, 2009. http://dx.doi.org/10.1063/1.3246447.

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Geiβler, K., M. R. Sterzik, G. Chauvin, E. Pantin, and Eric Stempels. "Mid-infrared imaging of brown dwarfs: Is HD 130948 BC variable?" In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099163.

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Karovicova, Iva, Markus Wittkowski, David A. Boboltz, Michael Scholz, and Eric Stempels. "Coordinated AMBER and MIDI observations of the Mira variable RR Aql." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099285.

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Semaan, T., C. Neiner, C. Martayan, et al. "Characterization and parameter determination of CoRoT variable stars with FLAMES." In STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION: Proceedings of the International Conference. AIP, 2009. http://dx.doi.org/10.1063/1.3246523.

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Schmidt, Edward G., Joyce Ann Guzik, and Paul A. Bradley. "Mining Sky Surveys for Astrophysically Interesting Variable Stars: The Cepheid Period Range." In STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION: Proceedings of the International Conference. AIP, 2009. http://dx.doi.org/10.1063/1.3246581.

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