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Relevant bibliographies by topics / Blue stragglers

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Academic literature on the topic 'Blue stragglers'

Author: Grafiati

Published: 4 June 2021

Last updated: 26 July 2025

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Journal articles on the topic "Blue stragglers"

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Jiang, Dengkai, Xuefei Chen, Lifang Li, and Zhanwen Han. "Binary evolution and double sequences of blue stragglers in globular clusters." Proceedings of the International Astronomical Union 14, S343 (2018): 427–28. http://dx.doi.org/10.1017/s1743921318005069.

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AbstractBinary evolution can produce different blue-straggler binaries, for example, blue stragglers with a bright, red component, or with a faint, blue component. In globular clusters, these blue-straggler binaries are generally observed as a single star, because two components can not be distinguished. Therefore, these blue-straggler binaries can be located in different regions of the color-magnitude diagram of globular clusters, e.g. blue sequence and red sequence observed in M30. We suggest that binary evolution can contribute to the blue stragglers in both of the sequences. Some blue stra

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Portegies Zwart, S. "The origin of the two populations of blue stragglers in M30." Astronomy & Astrophysics 621 (January 2019): L10. http://dx.doi.org/10.1051/0004-6361/201833485.

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We analyze the position of the two populations of blue stragglers in the globular cluster M30 in the Hertzsprung–Russell diagram. Both populations of blue stragglers are brighter than the cluster’s turn-off, but one population, the blue blue-stragglers, aligns along the zero-age main sequence whereas the other, red population is elevated in brightness (or color) by ∼0.75 mag. Based on stellar evolution and merger simulations we argue that the red population, which composes about 40% of the blue stragglers in M 30, has formed at a constant rate of ∼2.8 blue stragglers per gigayear over the last

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Leigh, Nathan, Alison Sills, and Christian Knigge. "Where the Blue Stragglers Roam: Searching for a Link Between Formation and Environment." Proceedings of the International Astronomical Union 3, S246 (2007): 331–35. http://dx.doi.org/10.1017/s1743921308015871.

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AbstractCurrent observational evidence seems to indicate that blue stragglers are a dynamically created population, though exactly how the mechanism(s) of formation operates remains a mystery. We search for links between blue straggler formation and environment by considering only those stars found within one core radius of the cluster center. In so doing, we aim to isolate a sample that is representative of an approximately uniform cluster environment where, ideally, a single blue straggler formation mechanism is predominantly operating. Normalized blue straggler frequencies are found and apa

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Pasquato, M. "FURTHER PROPERTIES OF THE DYNAMICAL CLOCK A+ INDICATOR IN A TOY MODEL OF PURE DYNAMICAL FRICTION." Revista Mexicana de Astronomía y Astrofísica 56, no. 1 (2020): 7–10. http://dx.doi.org/10.22201/ia.01851101p.2020.56.01.02.

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The Alessandrini A+ indicator is a measure of star cluster dynamical evolution based on the mass-segregation of blue straggler stars. A+ is defined as the integral of the cumulative distribution of blue stragglers over log radius, minus a term related to the reference population used. In a companion paper I introduced a model of dynamical friction and calculated the A+ indicator analytically. Here I show further properties of the time evolution of A+, focusing on the physical interpretation of its time derivative dA+ /dt. I find that dA+ /dt is the mean of the reciprocal dyamical friction time

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Chen, Xuefei, and Zhanwen Han. "Blue Stragglers from Primordial Binary Evolution." Proceedings of the International Astronomical Union 4, S252 (2008): 417–18. http://dx.doi.org/10.1017/s1743921308023351.

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AbstractBinaries exist in all clusters and much evidence suggests that close-binary evolution makes an important contribution to the blue straggler population, at least in some clusters as well as in the field. Here we present different channels to blue stragglers from primordial binary evolution and examine their contributions to the integrated spectral energy distribution of the host clusters in theory via binary population synthesis.

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Stryker, L. L. "Blue stragglers." Publications of the Astronomical Society of the Pacific 105 (October 1993): 1081. http://dx.doi.org/10.1086/133286.

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Rain, M. J., J. A. Ahumada, and G. Carraro. "A new, Gaia-based, catalogue of blue straggler stars in open clusters." Astronomy & Astrophysics 650 (June 2021): A67. http://dx.doi.org/10.1051/0004-6361/202040072.

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Context. Blue straggler stars are exotic objects present in all stellar environments whose nature and formation channels are still partially unclear. They seem to be particularly abundant in open clusters (OCs), thus offering a unique chance to tackle these problems statistically. Aims. We aim to build up a new and homogeneous catalogue of blue straggler stars (BSS) in Galactic OCs using Gaia to provide a more solid assessment of the membership of these stars. We also aim to explore possible relationships of the straggler abundance with the parent cluster’s structural and dynamical parameters.

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Nemec, James M., and Hugh C. Harris. "Evidence for Mass Segregation in NGC 5466." Symposium - International Astronomical Union 126 (1988): 677–78. http://dx.doi.org/10.1017/s0074180900043576.

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Forty-eight blue straggler stars have been discovered in NGC 5466, the only Galactic globular cluster known to contain an anomalous Cepheid of the sort found in dwarf galaxies. The stars were identified in color-magnitude diagrams constructed from photometry of deep photographic plates taken with the Canada-France-Hawaii 3.6 m telescope (calibrated with new UBV photoelectric photometry), and from point spread function photometry of CCD frames taken with the Palomar 5 m telescope. The stars typically have magnitudes <V> ~ 19.m1 and colors <B-V> ~ 0.m2. Forty-two of the 48 stars are

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Chen, Xuefei, and Zhanwen Han. "Primordial binary evolution and blue stragglers." Proceedings of the International Astronomical Union 5, S266 (2009): 333–38. http://dx.doi.org/10.1017/s1743921309991220.

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AbstractBlue stragglers have been found in all populations. They are important in both stellar evolution and stellar population synthesis. Much evidence shows that blue stragglers are relevant to primordial binaries. Here, we summarize the links between binary evolution and blue stragglers, describe the characteristics of blue stragglers originating from different binary evolutionary channels and show their consequences for binary population synthesis, such as for the integrated spectral-energy distribution, the colour–magnitude diagram, their specific frequency, and their influence on colours

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Dresbach, F., D. Massari, B. Lanzoni, et al. "Blue Stragglers as Tracers of the Dynamical State of Two Clusters in the Small Magellanic Cloud: NGC 339 and NGC 419." Astrophysical Journal 928, no. 1 (2022): 47. http://dx.doi.org/10.3847/1538-4357/ac5406.

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Abstract The level of central segregation of Blue Straggler stars has proved to be an excellent tracer of the dynamical evolution of old star clusters (the so-called “dynamical clock”), both in the Milky Way and in the Large Magellanic Cloud. The A + parameter, used to measure the Blue Stragglers degree of segregation, has in fact been found to strongly correlate with the parent cluster central relaxation time. Here, we have studied the Blue Straggler population of two young stellar systems in the Small Magellanic Cloud, namely NGC 339 (which is 6 Gyr old) and NGC 419 (with an age of only 1.5

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Dissertations / Theses on the topic "Blue stragglers"

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Ouellette, John Anders. "Blue stragglers." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 2000. http://www.collectionscanada.ca/obj/s4/f2/dsk2/ftp03/NQ47293.pdf.

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Venturi, Fulvia. "Un nuovo indicatore di segregazione radiale delle blue stragglers." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2016. http://amslaurea.unibo.it/9852/.

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Le blue straggler stars (BSS) sono un importante strumento osservativo per gli studi mirati alla determinazione dell'evoluzione dinamica degli ammassi globulari. La loro distribuzione radiale, influenzata dal fenomeno di segregazione di massa, costituisce un efficace strumento per la determinazione dello stato di rilassamento del sistema. In questo lavoro di tesi sono esplorate le potenzialità di un nuovo indicatore di segregazione centrale delle BSS: la cosiddetta "Area Positiva (A+)", definita come la differenza tra l'area sottesa dalla distribuzione radiale cumulativa delle BSS e quella di

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Andronov, Nikolay I. "Evolution of close binary stars with application to cataclysmic variables and Blue Stragglers." Connect to resource, 2005. http://rave.ohiolink.edu/etdc/view?acc%5Fnum=osu1126025974.

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Thesis (Ph. D.)--Ohio State University, 2005.<br>Title from first page of PDF file. Document formatted into pages; contains xii, 190 p.; also includes graphics (some col.). Includes bibliographical references (p. 181-190). Available online via OhioLINK's ETD Center.

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Santucci, Rafael Miloni. "Caracterização de estrelas azuis tardias no campo galáctico." Universidade de São Paulo, 2012. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-20062013-155903/.

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As estrelas azuis tardias (blue straggler stars ou estrelas BS) são estrelas de sequência principal que apresentam um aparente atraso evolutivo em relação às suas vizinhanças. Elas foram identificadas inicialmente na sequência principal de aglomerados globulares acima do ponto de turnoff no diagrama HR. Desde então, têm sido encontradas em todos os ambientes estelares: aglomerados abertos e globulares, galáxias anãs próximas e entre as estrelas de campo na Galáxia. O principal objetivo deste trabalho é construir uma grande amostra de estrelas BS no campo galáctico. Para tanto, métodos de sepa

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LAUZERAL, CEDRIC. "Observation de blue stragglers et photometrie de surface dans les regions centrales d'amas globulaires evolues dynamiquement." Toulouse 3, 1993. http://www.theses.fr/1993TOU30298.

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L'evolution dynamique des amas globulaires vers des densites centrales de plus en plus elevees conduit a l'effondrement de leur coeur. La presence d'un exces central de luminosite par rapport aux modeles stationnaires est associee a ce phenomene. Dans l'etude photometrique presentee, la contribution des etoiles brillantes est supprimee afin de reduire l'effet des erreurs d'echantillonnage et des biais eventuels sur les profils de luminance. Des diagrammes couleur-magnitude sont obtenus afin d'examiner le contenu stellaire. On rapporte la decouverte dans l'amas globulaire a coeur effondre ngc 6

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Dresbach, Francesca. "Lo stato dinamico di due ammassi stellari della Piccola Nube di Magellano tracciato dalla popolazione di Blue Stragglers." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amslaurea.unibo.it/22544/.

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Gli ammassi globulari sono sistemi stellari dinamicamente attivi, la cui struttura interna viene progressivamente modificata dalle frequenti interazioni gravitazionali tra le stelle che li compongono (evoluzione dinamica), su tempi scala difficilmente prevedibili. In queste condizioni si formano anche le Blue Straggler Stars, stelle caratterizzate da una massa più alta della media e quindi soggette all'azione della frizione dinamica, che le fa progressivamente migrare verso le zone centrali dell'ammasso. Lo studio di numerosi ammassi globulari vecchi, localizzati nella Via Lattea e nella Grand

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Andruet, Davide. "La popolazione di Blue Straggler Stars in due ammassi globulari della Grande Nube di Magellano." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2015. http://amslaurea.unibo.it/9650/.

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Le Blue Straggler Stars (BSS) sono la popolazione di oggetti esotici piu' comune e numerosa negli ammassi globulari. Nel diagramma colore-magnitudine le BSS definiscono una sequenza più brillante e blu del punto di turn-off della Sequenza Principale, simulando una popolazione più giovane delle stelle dell'ammasso. Osservazioni hanno dimostrato che le BSS hanno una massa significativamente più grande (1.2-1.7 Msun) di quella delle stelle di un ammasso globulare. Per questa proprietà, la distribuzione radiale delle BSS e' un utile strumento per tracciare empiricamente lo stato di evoluzione di

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Lattanzio, Daniele. "Analisi multi-diagnostica dello stato di evoluzione dinamica dell'ammasso globulare M15." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2020. http://amslaurea.unibo.it/20020/.

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Questo lavoro di tesi si inserisce nel contesto dello studio dell'evoluzione dinamica degli ammassi globulari. Essi sono dei sistemi collisionali, in cui le interazioni gravitazionali tra le stelle comportano continui scambi di energia cinetica tra le componenti di diversa massa. All'interno di questi ambienti molto densi, le frequenti interazioni possono arrivare a modificare profondamente le proprietà strutturali dell'ammasso. Infatti, sebbene gli ammassi globulari della Via Lattea abbiano tutti un’età cronologica molto simile, essi si sono evoluti dal punto di vista dinamico in maniera dive

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Murphy, Simon J., Maxwell Moe, Donald W. Kurtz, Timothy R. Bedding, Hiromoto Shibahashi, and Henri M. J. Boffin. "Finding binaries from phase modulation of pulsating stars with Kepler: V. Orbital parameters, with eccentricity and mass-ratio distributions of 341 new binaries." OXFORD UNIV PRESS, 2018. http://hdl.handle.net/10150/627133.

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The orbital parameters of binaries at intermediate periods (10(2)-10(3) d) are difficult to measure with conventional methods and are very incomplete. We have undertaken a new survey, applying our pulsation timing method to Kepler light curves of 2224 main-sequence A/F stars and found 341 non-eclipsing binaries. We calculate the orbital parameters for 317 PB1 systems (single-pulsator binaries) and 24 PB2s (double-pulsators), tripling the number of intermediate-mass binaries with full orbital solutions. The method reaches down to small mass ratios q approximate to 0.02 and yields a highly homog

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Royer, Frédéric. "Contribution à l'étude des populations d'étoiles chaudes à grande vitesse observées par Hipparcos." Phd thesis, Observatoire de Paris, 1999. http://tel.archives-ouvertes.fr/tel-00003537.

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Cette thèse est une étude de l'origine des étoiles chaudes à grande vitesse et/ou à grande distance du plan galactique, à l'aide des données du satellite Hipparcos. L'existence de ce type d'étoiles montre une incohérence entre le temps de vie assigné par la théorie de l'évolution stellaire aux étoiles de type B et A de Population I et celui beaucoup plus long des mécanismes responsables de l'augmentation de la dispersion des vitesses. Dans un premier temps, l'effet de la rotation stellaire sur les magnitudes absolues tirées des parallaxes trigonométriques est analysé sur un échantillon d'étoil

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Books on the topic "Blue stragglers"

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A, Saffer Rex, and Space Telescope Science Institute (U.S.), eds. Blue stragglers: Stars Journal Club Miniworkshop on Blue Stragglers held at the Space Telescope Science Institute, Baltimore, Maryland, 12-13 October 1992. Astronomical Society of the Pacific, 1993.

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E, Bond Howard, and United States. National Aeronautics and Space Administration, eds. UV observations of blue stragglers and population II K dwarfs: Final technical report, 1 July 1984 to 30 June 1986. National Aeronautics and Space Administration, 1987.

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Boffin, Henri M. J., Giovanni Carraro, and Giacomo Beccari, eds. Ecology of Blue Straggler Stars. Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44434-4.

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Stars Journal Club Miniworkshop on Blue Stragglers and Space Telescope Science Institute (U. S.). Blue Stragglers: Stars Journal Club Miniworkshop on Blue Stragglers Held at the Space Telescope Science Institute Baltimore, Maryland 12-13 October (Astronomical ... Society of the Pacific Conference Series). Astronomical Society of the Pacific, 1994.

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Boffin, Henri M. J., Giovanni Carraro, and Giacomo Beccari. Ecology of Blue Straggler Stars. Springer, 2016.

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Boffin, Henri M. J., Giovanni Carraro, and Giacomo Beccari. Ecology of Blue Straggler Stars. Springer, 2014.

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Boffin, Henri M. J., Giovanni Carraro, and Giacomo Beccari. Ecology of Blue Straggler Stars. Springer, 2014.

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Book chapters on the topic "Blue stragglers"

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Sills, Alison. "Models of Individual Blue Stragglers." In Ecology of Blue Straggler Stars. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-662-44434-4_12.

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Preston, George W. "Field Blue Stragglers and Related Mass Transfer Issues." In Ecology of Blue Straggler Stars. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-662-44434-4_4.

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Ivanova, Natalia. "Binary Evolution: Roche Lobe Overflow and Blue Stragglers." In Ecology of Blue Straggler Stars. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-662-44434-4_8.

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Chernyshova, Irina V. "Field Blue Stragglers: the Chemical Composition Revisited." In Chemical Evolution from Zero to High Redshift. Springer Berlin Heidelberg, 1999. http://dx.doi.org/10.1007/978-3-540-48360-1_11.

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Fischer, Daniel, and Hilmar Duerbeck. "Globular Clusters, White Dwarfs, and Blue Stragglers." In Hubble Revisited. Springer New York, 1998. http://dx.doi.org/10.1007/978-1-4612-2232-3_17.

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Knigge, Christian. "Blue Stragglers in Globular Clusters: Observations, Statistics and Physics." In Ecology of Blue Straggler Stars. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-662-44434-4_13.

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Mathieu, Robert D., and Aaron M. Geller. "The Blue Stragglers of the Old Open Cluster NGC 188." In Ecology of Blue Straggler Stars. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-662-44434-4_3.

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Xin, Yu, and Licai Deng. "Blue Stragglers in Clusters and Integrated Spectral Properties of Stellar Populations." In Ecology of Blue Straggler Stars. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-662-44434-4_14.

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Fischer, Daniel, and Hilmar Duerbeck. "Kugelsternhaufen, Weiße Zwerge und Blue Stragglers: Verjüngung durch Crash?" In Das Hubble-Universum. Birkhäuser Basel, 1998. http://dx.doi.org/10.1007/978-3-0348-6201-1_17.

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Da Costa, G. S., and John Norris. "Variability of ω Centauri Blue Stragglers: Clues to their Origin." In The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-015-1104-9_158.

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Conference papers on the topic "Blue stragglers"

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Holweger, Hartmut, Michael Lemke, Inga Rentzsch-Holm, and Sven Stürenburg. "Abundance patterns in unevolved A stars and in blue stragglers." In The 3rd international symposium on nuclear astrophysics: Nuclei in the Cosmos III. AIP, 1995. http://dx.doi.org/10.1063/1.47376.

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Chen, Xuefei, Zhanwen Han, Richard J. Stancliffe, Guenter Houdek, Rebecca G. Martin, and Christopher A. Tout. "Case C Mass Transfer and Long-orbital-period Blue Stragglers." In UNSOLVED PROBLEMS IN STELLAR PHYSICS: A Conference in Honor of Douglas Gough. AIP, 2007. http://dx.doi.org/10.1063/1.2819005.

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Mathieu, Robert D., Vicky Kologera, and Marc van der Sluys. "The Blue Stragglers: At the Interface of Stellar Evolution and Stellar Dynamics." In INTERNATIONAL CONFERENCE ON BINARIES: In celebration of Ron Webbink’s 65th Birthday. AIP, 2010. http://dx.doi.org/10.1063/1.3536423.

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Arbutina, Bojan, and Surjit Wadhwa. "THE CRITICAL MASS RATIO FOR W UMA-TYPE CONTACT BINARIES." In XIV Serbian-Bulgarian Astronomical Conference. Astronomical Observatory, 2024. http://dx.doi.org/10.69646/14sbac11a.

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W UMa-type contact binaries are close binary systems of low mass in which both components fill their inner Roche lobes. Low mass ratio systems of this type are especially interesting because there are indications that in their case components can merge and form fast- rotating stars such as FC Com stars and the blue-stragglers, and (luminous) red novae such as V1309 Sco. The condition for the onset of tidal (Darwin) instability and probable merger can be linked to some critical mass ratio below which we expect a contact system to be unstable. We give an overview of this condition and show how i

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Sills, Alison, Vicky Kologera, and Marc van der Sluys. "Blue Straggler Formation in Clusters." In INTERNATIONAL CONFERENCE ON BINARIES: In celebration of Ron Webbink’s 65th Birthday. AIP, 2010. http://dx.doi.org/10.1063/1.3536351.

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Glebbeek, Evert, Alison Sills, Haili Hu, Richard J. Stancliffe, Vicky Kologera, and Marc van der Sluys. "Blue Straggler Surface Abundances: A Clue to Their Formation History?" In INTERNATIONAL CONFERENCE ON BINARIES: In celebration of Ron Webbink’s 65th Birthday. AIP, 2010. http://dx.doi.org/10.1063/1.3536352.

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Gosnell, Natalie. "Blue Straggler Stars: A Window Into Alternative Pathway Stellar Products." In Frank N. Bash Symposium 2015. Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.261.0005.

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Leigh, Nathan, Alison Sills, Vicky Kologera, and Marc van der Sluys. "Stellar Encounters with Multiple Star Systems and the Blue Straggler Problem." In INTERNATIONAL CONFERENCE ON BINARIES: In celebration of Ron Webbink’s 65th Birthday. AIP, 2010. http://dx.doi.org/10.1063/1.3536353.

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