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Relevant bibliographies by topics / Stellar dynamics and kinematics

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Academic literature on the topic 'Stellar dynamics and kinematics'

Author: Grafiati

Published: 17 September 2021

Last updated: 10 March 2023

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Journal articles on the topic "Stellar dynamics and kinematics"

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Bonfanti, P., F. Simien, R. Rampazzo, and Ph Prugniel. "Kinematics of early-type galaxies in compact groups: HCG 67, HCG 74 and HCG 79." International Astronomical Union Colloquium 174 (2000): 50–53. http://dx.doi.org/10.1017/s0252921100054749.

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AbstractWe present measurements of stellar kinematics for seven early-type galaxies in HCG 67, HCG 74 and HCG 79. These data are aimed at studying the relation between the environment and the dynamics, structure and stellar content of early-type galaxies. In the present three groups, the kinematic features we observed cannot be associated unambiguously to physical interactions. Visible morphological peculiarities do not appear correlated with kinematical perturbations.

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Zeeuw, Tim De. "Dynamics of the Galactic Bulge." Symposium - International Astronomical Union 153 (1993): 191–208. http://dx.doi.org/10.1017/s0074180900123198.

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Recent work on the intrinsic shape, the internal kinematics of stars and gas, and the dynamics of the Galactic Bulge is discussed. Starcounts, measurements of the integrated light and the kinematics of the atomic and molecular gas all provide strong evidence that the Bulge is triaxial, and is rotating fairly rapidly. To date, there is little evidence for triaxiality in the stellar kinematics: the available stellar velocities are consistent with Kent's (1992) oblate model. This unsatisfactory situation is expected to improve rapidly.

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Yttergren, M., P. Misquitta, Á. Sánchez-Monge, et al. "Gas and stellar dynamics in Stephan’s Quintet." Astronomy & Astrophysics 656 (December 2021): A83. http://dx.doi.org/10.1051/0004-6361/202040188.

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In nearby compact galaxy groups we can study the complex processes of galaxy interactions at high resolution and obtain a window into a time in the history of the Universe when the galaxies were closely spaced and the intergalactic medium was awash with gas. Stephan’s Quintet is a nearby compact galaxy group and a perfect laboratory for studying the process of galaxy evolution through galaxy harassment and interaction. By analysing the kinematics of Stephan’s Quintet we aim to provide an increased understanding of the group, the history of the interactions, their cause and effect, and the deta

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van der Marel, Roeland P. "Recent Progress in the Search for Black Holes in Galactic Nuclei." Symposium - International Astronomical Union 171 (1996): 117–20. http://dx.doi.org/10.1017/s0074180900232233.

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Massive nuclear black holes (BHs) of 106–109M⊙ are believed to be responsible for the the energy production in quasars and active galaxies, and are thought to be present in many quiescent galaxies as well. Dynamical evidence for this can be sought by studying the dynamics of gas and stars in galactic nuclei at high spatial resolution. This paper reviews the current evidence, with emphasis on some recent developments and ongoing projects. The evidence from water masers and gas kinematics in the active galaxies NGC 4258 and M87 is compelling. In quiescent galaxies only stellar kinematics are gen

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Dejonghe, H., P. Vauterin, K. Van Caelenberg, S. Durand, and A. Mathieu. "Kinematics and dynamics of galactic systems as probed by Planetary Nebulae samples." Symposium - International Astronomical Union 180 (1997): 428–37. http://dx.doi.org/10.1017/s0074180900131687.

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At the current epoch, the dynamics of galactic systems is largely controlled by the behaviour of the stellar component. There is probably also a large amount of non-stellar matter present, which probably dominates the dynamics on large scales. Nevertheless, the (centers of) galaxies are still, for better or worse, defined as those regions were there happens to be a lot of stellar light.

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Tsukui, Takafumi, Satoru Iguchi, and Kyoko Onishi. "Galactic dynamics and DM profile of NGC1380 with ALMA and VLT/MUSE." Proceedings of the International Astronomical Union 14, S353 (2019): 248–52. http://dx.doi.org/10.1017/s1743921319008767.

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AbstractIn order to understand the interaction between dark matter and baryonic matter in the galaxy evolution history, it is fundamental to constrain dark matter (DM) distribution in galaxies. However, it is difficult to constrain DM profile in the central region of early type galaxy because of the lack of extended neutral hydrogen gas and the degeneracy between dynamical stellar M/L and DM profile. To resolve this difficulty, we conducted combined analysis of ALMA cold molecular gas kinematics and MUSE stellar kinematics of early type fast rotator galaxy NGC1380. In addition, we used HST ima

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Tiongco, Maria A., Enrico Vesperini, and Anna Lisa Varri. "Kinematical evolution of multiple stellar populations in star clusters." Monthly Notices of the Royal Astronomical Society 487, no. 4 (2019): 5535–48. http://dx.doi.org/10.1093/mnras/stz1595.

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ABSTRACT We present the results of a suite of N-body simulations aimed at understanding the fundamental aspects of the long-term evolution of the internal kinematics of multiple stellar populations in globular clusters. Our models enable us to study the cooperative effects of internal, relaxation-driven processes and external, tidally induced perturbations on the structural and kinematic properties of multiple-population globular clusters. To analyse the dynamical behaviour of the multiple stellar populations in a variety of spin-orbit coupling conditions, we have considered three reference ca

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Barnabè, Matteo, Chiara Spiniello, and Léon V. E. Koopmans. "Dissecting the 3D structure of elliptical galaxies with gravitational lensing and stellar kinematics." Proceedings of the International Astronomical Union 10, S309 (2014): 77–80. http://dx.doi.org/10.1017/s1743921314009351.

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AbstractThe combination of strong gravitational lensing and stellar kinematics provides a powerful and robust method to investigate the mass and dynamical structure of early-type galaxies. We demonstrate this approach by analysing two massive ellipticals from the XLENS Survey for which both high-resolution HST imaging and X-Shooter spectroscopic observations are available. We adopt a flexible axisymmetric two-component mass model for the lens galaxies, consisting of a generalised NFW dark halo and a realistic self-gravitating stellar mass distribution. For both systems, we put constraints on t

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Straatman, Caroline M. S., Arjen van der Wel, Josha van Houdt, et al. "LEGA-C: Analysis of Dynamical Masses from Ionized Gas and Stellar Kinematics at z ∼ 0.8." Astrophysical Journal 928, no. 2 (2022): 126. http://dx.doi.org/10.3847/1538-4357/ac4e18.

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Abstract We compare dynamical mass estimates based on spatially extended stellar and ionized gas kinematics (M dyn,* and M dyn,eml, respectively) of 157 star-forming galaxies at 0.6 ≤ z < 1. Compared with z ∼ 0, these galaxies have enhanced star formation rates, with stellar feedback likely affecting the dynamics of the gas. We use LEGA-C DR3, the highest-redshift data set that provides sufficiently deep measurements of a K s -band limited sample. For M dyn,*, we use Jeans anisotropic multi-Gaussian expansion models. For M dyn,eml, we first fit a custom model of a rotating exponential disk

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Gerhard, Ortwin, James Binney, and Hongsheng Zhao. "The Galactic Bar." Highlights of Astronomy 11, no. 2 (1998): 628–34. http://dx.doi.org/10.1017/s1539299600018293.

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AbstractWe summarize recent work on the structure and dynamics of the Galactic bar and inner disk. Current work focusses on constructing a quantitative model which integrates NIR photometry, source count observations, gas kinematics, stellar dynamical observations, and microlensing. Some avenues for future research are discussed.

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Dissertations / Theses on the topic "Stellar dynamics and kinematics"

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Sperauskas, J., S. Bartašiūtė, R. P. Boyle, V. Deveikis, S. Raudeliūnas, and A. R. Upgren. "Radial velocities of K–M dwarfs and local stellar kinematics." EDP SCIENCES S A, 2016. http://hdl.handle.net/10150/622691.

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Aims. The goal of this paper is to present complete radial-velocity data for the spectroscopically selected McCormick sample of nearby K-M dwarfs and, based on these and supplementary data, to determine the space-velocity distributions of late-type stars in the solar neighborhood. Methods. We analyzed nearly 3300 measurements of radial velocities for 1049 K-M dwarfs, that we obtained during the past decade with a CORAVEL-type instrument, with a primary emphasis on detecting and eliminating from kinematic calculations the spectroscopic binaries and binary candidates. Combining radial-velocity d

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Da, Rio Nicola, Jonathan C. Tan, Kevin R. Covey, et al. "IN-SYNC. V. Stellar Kinematics and Dynamics in the Orion A Molecular Cloud." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/625776.

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The kinematics and dynamics of young stellar populations enable us to test theories of star formation. With this aim, we continue our analysis of the SDSS-III/APOGEE IN-SYNC survey, a high-resolution near-infrared spectroscopic survey of young clusters. We focus on the Orion A star-forming region, for which IN-SYNC obtained spectra of similar to 2700 stars. In Paper IV we used these data to study the young stellar population. Here we study the kinematic properties through radial velocities (vr). The young stellar population remains kinematically associated with the molecular gas, following a s

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Silva, Manuel Duarte de Vasconcelos. "Runaway stars in the Galactic halo : their origin and kinematics." Thesis, University of Hertfordshire, 2012. http://hdl.handle.net/2299/8115.

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Star formation in the Milky Way is confined to star-forming regions (OB association, HII regions, and open clusters) in the Galactic plane. It is usually assumed that these regions are found preferably along spiral arms, as is observed in other spiral galaxies. However, young early-type stars are often found at high Galactic latitudes, far away from their birthplaces in the Galactic disc. These stars are called runaway stars, and it is believed that they were ejected from their birth- places early in their lifetimes by one of two mechanisms: ejection from a binary system following the destruct

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Khanna, Shourya. "The GALAH and GAIA surveys: the response of the Galactic disk to non-equilibrium features." Thesis, The University of Sydney, 2019. https://hdl.handle.net/2123/21641.

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The dynamical history of the Milky Way is complicated. We see a lot of substructure (that is likely accreted), both in spatial density, and in kinematics. The complexity varies, from simple streams to phase-mixed structures that can only be separated by invariants such as stellar chemistry. To complicate things further, the Galaxy has non-axisymmetric structures such as the bar and multiple spiral arms. Due to their large scale-lengths, the kinematic signatures of such features often overlap, making it difficult to relate to one culprit or another. With the aid of high precision spectroscopy a

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Barbosa, Carlos Eduardo. "Kinematics and stellar populations of galaxies in the local universe." Universidade de São Paulo, 2016. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-22042018-235533/.

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Galaxies are the major building blocks of the universe, but we are still learning about fundamental aspects of their formation. In particular, we would like to understand how galaxies acquire their stars, and where and when these stars were born. In this thesis, we investigate these questions by the study of the dynamical and chemical abundances of galaxies in the local universe. Extending previous works in the field, we have developed a Bayesian framework to obtain luminosity-weighted ages, metallicities and alpha-element abundances. In our initial study, we have surveyed six galaxy groups to

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Fermani, Francesco. "Modelling the Milky Way stellar halo." Thesis, University of Oxford, 2013. http://ora.ox.ac.uk/objects/uuid:bcd70530-506d-46c2-8c99-7f5b8f08f915.

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We motivate the importance of understanding the kinematics and dynamics of the Milky Way stellar halo both in unravelling the formation history and evolution of our host Galaxy and in the more general context of galaxy dynamics. We present a cleaned picture of the kinematics of the smooth component of the stellar halo: we develop a method to quantify the average distance error on a sample of stars based on the idea of Schoenrich et al. (2012), but adapted so that it uses velocity information only on average. We use this scheme to construct an analytic distance calibration for Blue Horizontal B

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ZOCCHI, ALICE. "OBSERVATIONAL TESTS ON THE DYNAMICS OF GLOBULAR CLUSTERS." Doctoral thesis, Università degli Studi di Milano, 2014. http://hdl.handle.net/2434/235122.

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Galactic globular clusters are nearly gas-free, self-gravitating stellar systems characterized by an apparently simple geometry, with finite size probably determined by tidal truncation. These unique properties make them excellent laboratories for studies of stellar dynamics, and ideal targets for N-body simulations. For a long time, they have been treated as spherically symmetric, nonrotating, isotropic systems. The spherical King (1966) models, constructed to match this physical picture, are usually considered as the correct zeroth-order dynamical reference model, and are sometimes successfu

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Sohn, Sangmo Tony, der Marel Roeland P. van, Nitya Kallivayalil, et al. "HUBBLE SPACE TELESCOPE PROPER MOTIONS OF INDIVIDUAL STARS IN STELLAR STREAMS: ORPHAN, SAGITTARIUS, LETHE, AND THE NEW “PARALLEL STREAM”." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/622680.

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We present a multi-epoch Hubble Space Telescope (HST) study of stellar proper motions (PMs) for four fields along the Orphan Stream. We determine absolute PMs of several individual stars per target field using established techniques that utilize distant background galaxies to define a stationary reference frame. Five Orphan Stream stars are identified in one of the four fields based on combined color-magnitude and PM information. The average PM is consistent with the existing model of the Orphan Stream by Newberg et al. In addition to the Orphan Stream stars, we detect stars that likely belong

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Besla, Gurtina, David Martínez-Delgado, der Marel Roeland P. van, et al. "LOW SURFACE BRIGHTNESS IMAGING OF THE MAGELLANIC SYSTEM: IMPRINTS OF TIDAL INTERACTIONS BETWEEN THE CLOUDS IN THE STELLAR PERIPHERY." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621396.

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We present deep optical images of the Large and Small Magellanic Clouds (LMC and SMC) using a low cost telephoto lens with a wide field of view to explore stellar substructure in the outskirts of the stellar disk of the LMC (< 10 degrees from the LMC center). These data have higher resolution than existing star count maps, and highlight the existence of stellar arcs and multiple spiral arms in the northern periphery, with no comparable counterparts in the south. We compare these data to detailed simulations of the LMC disk outskirts, following interactions with its low mass companion, the SMC.

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Marchetto, Alina. "The Solar System dynamical interaction with the Galaxy environment: evolutionary implications for alien Oort clouds and exo-planets." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2022. http://amslaurea.unibo.it/25369/.

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The Sun is located in the Orion Arm of the Milky Way galaxy and its surrounded, along with other bodies, by stars. This thesis work aims at understanding whether these stars can dynamically interact with the Sun and its Solar System and to investigate the possible features of this kind of interactions. We will begin from an observable quantity, the Oort surface density for stars, and we will build a stellar density profile for the Milky Way galaxy using the model suggested by Juric et al., 2008. Then, making use of the Initial Mass Function and the Star Formation Rate function, we will calcula

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Books on the topic "Stellar dynamics and kinematics"

1

Cubarsi, Rafael. Kinematics and dynamics of galactic stellar populations. Cambridge Scholars Publishing, 2018.

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Bottema, Roelof. The stellar kinematics of galactic disks. Rijksuniversiteit Groningen,c1995., 1995.

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Schwinger, Julian Seymour. Quantum kinematics and dynamics. Addison-Wesley Pub. Co. Advanced Book Program, 1991.

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Schwinger, Julian Seymour. Quantum Kinematics and Dynamics. Advanced Book Program, Perseus Pub., 2000.

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Huston, Ronald L. Multibody dynamics. Butterworths, 1990.

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Huston, Ronald L. Multibody dynamics. Butterworth-Heinemann, 1990.

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Huston, Ronald L. Multibody dynamics. Butterworths, 1990.

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J, Thompson M., and Christensen-Dalsgaard Jørgen 1950-, eds. Stellar astrophysical fluid dynamics. Cambridge University Press, 2003.

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Peter, Sadler J., ed. Kinematics and dynamics of machinery. 2nd ed. HarperCollinsCollegePublishers, 1993.

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Kinematics and dynamics of machinery. M. Dekker, 1996.

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Book chapters on the topic "Stellar dynamics and kinematics"

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Davies, Roger L. "The Stellar Kinematics of Elliptical Galaxies." In Structure and Dynamics of Elliptical Galaxies. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3971-4_5.

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Wielen, Roland. "Structure, Kinematics and Dynamics of Stellar Systems." In Gesammelte Werke Collected Works. Springer Berlin Heidelberg, 1992. http://dx.doi.org/10.1007/978-3-642-58086-4_6.

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Raga, A. C. "Coupled Stellar Jet/Molecular Outflow Models." In Kinematics and Dynamics of Diffuse Astrophysical Media. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0926-0_16.

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Sommer-Larsen, Jesper. "Kinematics and Dynamics of the Galactic Stellar Halo." In Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4213-7_20.

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Reid, I. Neill. "Stellar Kinematics and the Dynamical Evolution of the Disc." In Dynamics of Young Star Clusters and Associations. Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-47290-3_17.

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Runacres, M., and R. Blomme. "The Importance of Continuum Radiation for the Stellar Wind Hydrodynamics of Hot Stars." In Kinematics and Dynamics of Diffuse Astrophysical Media. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0926-0_10.

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Smart, R. L. "Kinematics of Orion Association Members." In Stellar Populations. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0125-7_49.

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Nezhinskij, E. M., L. P. Ossipkov, and S. A. Kutuzov. "Open Cluster System: Kinematics, Orbits." In Stellar Populations. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0125-7_50.

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Wittenburg, Jens. "Dynamics of Mechanisms." In Kinematics. Springer Berlin Heidelberg, 2016. http://dx.doi.org/10.1007/978-3-662-48487-6_19.

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Fabien, Brian. "Kinematics." In Analytical System Dynamics. Springer US, 2008. http://dx.doi.org/10.1007/978-0-387-85605-6_2.

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Conference papers on the topic "Stellar dynamics and kinematics"

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Mickaelian, A. M., G. A. Mikayelyan, H. V. Abrahamyan, and G. M. Paronyan. "Discovery and study of new white dwarfs by means of Gaia EDR3 accurate astrometry." In ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.189.

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The discovery and study of new White Dwarfs (WDs) is extremely important for understanding the kinematics and dynamicsof the local stellar population. They are evolutionary signatures of the Milky Way, as most of stars pass through thisevolutionary stage. We have carried out a statistical analysis of the White Dwarfs Catalogue to establish their averagephysical properties. Based on these data, we have searched for new WDs using Gaia EDR3 accurate astrometry. It provideshuge amount of data to conﬁrm WDs and reveal many more such objects. Gaia’s astrometric accuracy allows more detailedstudies o

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González Delgado, Rosa M., Claus Leitherer, and Timothy Heckman. "Stellar content and kinematics of starburst galaxies." In The ultraviolet universe at low and high redshift. AIP, 1997. http://dx.doi.org/10.1063/1.53742.

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Kokkotas, K. D. "Stellar Dynamics in Scalar-Tensor Gravity." In RECENT ADVANCES IN ASTRONOMY AND ASTROPHYSICS: 7th International Conference of the Hellenic Astronomical Society. AIP, 2006. http://dx.doi.org/10.1063/1.2348058.

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Cappellari, Michele, Richard M. McDermid, R. Bacon, et al. "Testing Mass Determinations of Supermassive Black Holes via Stellar Kinematics." In HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458489.

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McGinn, M. T., K. Sellgren, E. E. Becklin, D. N. B. Hall, and I. Gatley. "Stellar kinematics in the central 10 pc of the galaxy." In AIP Conference Proceedings Volume 155. AIP, 1987. http://dx.doi.org/10.1063/1.36405.

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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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Trujillo, Ignacio, Judit Bakos, Victor P. Debattista, and C. C. Popescu. "Stellar Disk Truncations: HI Density and Dynamics." In HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458507.

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Vinko, J., Laszlo B. Kish, G. Kaszas, and G. Furesz. "Application of optical spectroscopy in stellar dynamics." In OPTIKA '98: Fifth Congress on Modern Optics, edited by Gyorgy Akos, Gabor Lupkovics, and Andras Podmaniczky. SPIE, 1998. http://dx.doi.org/10.1117/12.321024.

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Bauer, W., T. Strother, Ricardo Alarcon, Philip L. Cole, Chaden Djalali, and Fernando Umeres. "Nuclear Reactions and Stellar Evolution: Unified Dynamics." In VII Latin American Symposium on Nuclear Physics and Applications. AIP, 2007. http://dx.doi.org/10.1063/1.2813827.

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El-Khasawneh, Bashar, and Anas Alazzam. "Kinematics, Dynamics and Vibration Models for 3RPR Parallel Kinematics Manipulator." In ASME 2013 International Mechanical Engineering Congress and Exposition. American Society of Mechanical Engineers, 2013. http://dx.doi.org/10.1115/imece2013-64525.

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Parallel link manipulators are the type of mechanisms that have closed kinematics chains. Some of their advantages over open kinematics chains (called also serial kinematics manipulators) are their high stiffness and accuracy. This paper carries out forward and inverse kinematic and dynamic analysis on a certain type of parallel kinematic mechanisms. This is needed to conduct vibration analysis on the same platform. The type of mechanism is planar 3 RPR manipulator. This entails identifying the modes of the manipulator. A simplified vibration theoretical model is derived. This derivation helps

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Reports on the topic "Stellar dynamics and kinematics"

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Aardema, James. Robotic Refueler Arm Kinematics, Dynamics and Global Position Control. Defense Technical Information Center, 1989. http://dx.doi.org/10.21236/ada396690.

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Keyser, Daniel. Diagnosis of the Kinematics and Dynamics of Rapidly Developing Maritime Cyclones. Defense Technical Information Center, 1992. http://dx.doi.org/10.21236/ada267008.

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Chou, W., C. T. Tajima, R. Matsumoto, and K. Shibata. Dynamics of local isolated magnetic flux tubes in a fast-rotating stellar atmosphere. Office of Scientific and Technical Information (OSTI), 1998. http://dx.doi.org/10.2172/585017.

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Melville, W. K., and Eric Terrill. Airborne Measurements of Whitecap Kinematics and Dynamics in the High-Wind Regime: Source Functions for Marine Aerosols, Surface Currents and Turbulence. Defense Technical Information Center, 2003. http://dx.doi.org/10.21236/ada630299.

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Kozlovsky, Evgen O., та Hennadiy M. Kravtsov. Мультимедийная виртуальная лаборатория по физике в системе дистанционного обучения. [б. в.], 2018. http://dx.doi.org/10.31812/0564/2455.

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Research goals: the description of technology of software development in Physics Virtual Laboratory for Distance Learning System. Research objectives: the architecture of client and server parts of the lab, the functionality of the system modules, user roles, as well as the principles of virtual laboratory use on a personal computer. Object of research: the distance learning system “Kherson Virtual University”. Subject of research: virtual laboratory for physics in the distance learning. Research methods used: analysis of statistics and publications. Results of the research. The development of

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