Relevant bibliographies by topics / Galaxy: centre

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Galaxy: centre'

Author: Grafiati
Published: 4 June 2021
Last updated: 21 December 2024

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Journal articles on the topic "Galaxy: centre"

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Bellovary, Jillian M., Sarra Hayoune, Katheryn Chafla, et al. "The origins of off-centre massive black holes in dwarf galaxies." Monthly Notices of the Royal Astronomical Society 505, no. 4 (2021): 5129–41. http://dx.doi.org/10.1093/mnras/stab1665.

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ABSTRACT Massive black holes often exist within dwarf galaxies, and both simulations and observations have shown that a substantial fraction of these may be off-centre with respect to their hosts. We trace the evolution of off-centre massive black holes (MBHs) in dwarf galaxies using cosmological hydrodynamical simulations, and show that the reason for off-centre locations is mainly due to galaxy–galaxy mergers. We calculate dynamical time-scales and show that off-centre MBHs are unlikely to sink to their galaxys’ centres within a Hubble time, due to the shape of the hosts’ potential wells and
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Yan, Z., N. Raza, L. Van Waerbeke, et al. "An analysis of galaxy cluster mis-centring using cosmological hydrodynamic simulations." Monthly Notices of the Royal Astronomical Society 493, no. 1 (2020): 1120–29. http://dx.doi.org/10.1093/mnras/staa295.

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ABSTRACT The location of a galaxy cluster’s centroid is typically derived from observations of the galactic and/or gas component of the cluster, but these typically deviate from the true centre. This can produce bias when observations are combined to study average cluster properties. Using data from the BAryons and HAloes of MAssive Systems (BAHAMAS) cosmological hydrodynamic simulations, we study this bias in both two and three dimensions for 2000 clusters over the 1013–1015 M⊙ mass range. We quantify and model the offset distributions between observationally motivated centres and the ‘true’
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Clube, S. V. M., and R. Pan. "The kinematic centre of the Galaxy." Monthly Notices of the Royal Astronomical Society 216, no. 3 (1985): 511–19. http://dx.doi.org/10.1093/mnras/216.3.511.

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Gerhard, Ortwin E. "Dynamics of the Bar at the Galactic Centre." Symposium - International Astronomical Union 169 (1996): 79–91. http://dx.doi.org/10.1017/s0074180900229550.

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There is now substantial evidence for a rotating bar in the inner Galaxy. This is an important change in our perception of the Galaxy because it changes the ways in which we have to think about its evolutionary history.
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Simatupang, Yosua. "Redesign of the Galaxy Gym Tembung Logo as Brand Identity." Jurnal Indonesia Sosial Sains 5, no. 06 (2024): 1534–44. http://dx.doi.org/10.59141/jiss.v5i06.1160.

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Competition in the fitness centre industry is getting tighter. This encourages Galaxy Gym Tembung to improve its brand identity in order to compete with its competitors. One of the efforts made is to redesign the logo. Galaxy Gym Tembung which is located in the area of Jalan Moh. Yakub Lubis No.dsn 3, Bandar Khalipah, Percut Sei Tuan District, Deli Serdang Regency, East Medan District, which was established in 2019, is one of the fitness centres located in Tembung with its owner named Ridho Santoso. This research aims to improve the brand identity of Galaxy Gym Tembung as a fitness centre. Thi
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Coleman, M. G., and G. S. Da Costa. "A Second Shell in the Fornax dSph Galaxy." Publications of the Astronomical Society of Australia 22, no. 2 (2005): 162–65. http://dx.doi.org/10.1071/as04067.

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AbstractIn the search for tidal structure in Galactic satellite systems, we have conducted a photometric survey over a 10 deg2 area centred on the Fornax dSph galaxy. The survey was made in two colours, and the resulting colour–magnitude data were used as a mask to select candidate Fornax RGB stars, thereby increasing the contrast of Fornax stars to background sources in the outer regions. Previously, we reported the presence of a shell (age 2 Gyr) located towards the centre of Fornax. In this contribution we reveal a second shell, significantly larger than the first, located 1.3° north-west f
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Netchitailo, Vladimir S. "Hypersphere World-Universe Model: Centre of Our Galaxy." Journal of High Energy Physics, Gravitation and Cosmology 08, no. 01 (2022): 25–55. http://dx.doi.org/10.4236/jhepgc.2022.81003.

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Morris, Mark. "What's happening at the centre of our galaxy?" Physics World 7, no. 10 (1994): 37–43. http://dx.doi.org/10.1088/2058-7058/7/10/30.

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Battersby, Stephen. "The monster at the centre of the galaxy." New Scientist 202, no. 2709 (2009): 28–31. http://dx.doi.org/10.1016/s0262-4079(09)61388-9.

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Knebe, Alexander, Matías Gámez-Marín, Frazer R. Pearce, et al. "The Three Hundred project: shapes and radial alignment of satellite, infalling, and backsplash galaxies." Monthly Notices of the Royal Astronomical Society 495, no. 3 (2020): 3002–13. http://dx.doi.org/10.1093/mnras/staa1407.

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ABSTRACT Using 324 numerically modelled galaxy clusters, we investigate the radial and galaxy–halo alignment of dark matter subhaloes and satellite galaxies orbiting within and around them. We find that radial alignment depends on distance to the centre of the galaxy cluster but appears independent of the dynamical state of the central host cluster. Furthermore, we cannot find a relation between radial alignment of the halo or galaxy shape with its own mass. We report that backsplash galaxies, i.e. objects that have already passed through the cluster radius but are now located in the outskirts
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Dissertations / Theses on the topic "Galaxy: centre"

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Nieuwmunster, Niels. "Les systèmes les plus denses de l'Univers : le disque nucléaire." Electronic Thesis or Diss., Université Côte d'Azur, 2024. http://www.theses.fr/2024COAZ5041.

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Comprendre la formation et l'évolution des galaxies, et en particulier de leurs centres galactiques, est l'une des questions les plus intrigantes de l'astrophysique moderne. De nombreuses galaxies spirales comme la Voie lactée présentent en leur centre un disque nucléaire (NSD). Celui de la Voie lactée est, avec l'amas central et le trou noir super massif central, l'une des principales composantes internes et l'un des meilleurs laboratoires locaux disponibles pour étudier l'évolution des galaxies. En raison de la forte extinction, de l'importante densité d'étoiles et de la superposition de mul
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Blank, M., M. R. Morris, A. Frank, J. J. Carroll-Nellenback, and W. J. Duschl. "The inner cavity of the circumnuclear disc." OXFORD UNIV PRESS, 2016. http://hdl.handle.net/10150/617417.

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The circumnuclear disc (CND) orbiting the Galaxy's central black hole is a reservoir of material that can ultimately provide energy through accretion, or form stars in the presence of the black hole, as evidenced by the stellar cluster that is presently located at the CND's centre. In this paper, we report the results of a computational study of the dynamics of the CND. The results lead us to question two paradigms that are prevalent in previous research on the Galactic Centre. The first is that the disc's inner cavity is maintained by the interaction of the central stellar cluster's strong wi
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Dexter, J., A. Deller, G. C. Bower, et al. "Locating the intense interstellar scattering towards the inner Galaxy." OXFORD UNIV PRESS, 2017. http://hdl.handle.net/10150/625730.

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We use VLBA+VLA observations to measure the sizes of the scatter-broadened images of six of the most heavily scattered known pulsars: three within the Galactic Centre (GC) and three elsewhere in the inner Galactic plane (Delta l < 20 degrees). By combining the measured sizes with temporal pulse broadening data from the literature and using the thin-screen approximation, we locate the scattering medium along the line of sight to these six pulsars. At least two scattering screens are needed to explain the observations of the GC sample. We show that the screen inferred by previous observations of
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Rees, Bryan. "A study of planetary nebulae in and towards the Galactic Bulge." Thesis, University of Manchester, 2011. https://www.research.manchester.ac.uk/portal/en/theses/a-study-of-planetary-nebulae-in-and-towards-the-galactic-bulge(ff6c0373-e5a5-491f-b5fb-bda36acac8ba).html.

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A planetary nebula (PN) consists of material, mainly gas, that has been ejected from a star on the asymptotic giant branch of its life cycle. This material emits electromagnetic radiation due to photoionization and recombination, collisional and radiative excitation or free-free radiation. The envelope of material moves outwards from the central star and may take one of a variety of shapes. These shapes are believed to be sculpted by the stellar wind, magnetic fields and interactions with a binary companion. However, within a time scale of as little as 10 000 years the nebula fades from view a
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Ciurlo, Anna. "Physical and dynamical conditions of the molecular gas in the central parsec of the Galaxy." Sorbonne Paris Cité, 2015. https://theses.hal.science/tel-01540979.

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Dans le parsec central de la Galaxie l'environnement du trou noir (Sgr A*) présente un cluster d'étoiles jeunes et deux structures de gaz : le Disque Circumnucléaire, moléculaire, et la Minispirale, ionisée. Nous avons investigué la présence du gaz neutre dans la cavité centrale du CND, où s'étale la Minispirale, pour décrire la distribution et les propriétés du H2 dans cet environnement ionisé. Cette étude a été menée à travers un cube de données de spectro-imagerie en infrarouge proche, observé par SPIFF1 au VLT. Pour conserver la résolution spatiale et éviter les effets de bords nous avons
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Lucas, William. "Gas flow and star formation in the centre of the Milky Way : investigations with smoothed particle hydrodynamics." Thesis, University of St Andrews, 2015. http://hdl.handle.net/10023/6601.

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The centre of the Milky Way, commonly referred to as the Galactic Centre, is roughly that region within 500 pc of the central black hole, Sagittarius A*. Within the innermost parsec around the supermassive black hole Sagittarius A* are more than a hundred massive young stars whose orbits align to form one or possibly two discs. At about 100 pc is a ring containing more than ten million solar masses of molecular gas which could be the origin of some of the most massive star clusters in the Galaxy. I have performed a number of numerical simulations to help us understand how it is that these stru
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Nandakumar, Govind. "L’archéologie galactique et son application au centre galactique." Thesis, Université Côte d'Azur (ComUE), 2018. http://www.theses.fr/2018AZUR4064/document.

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L'archéologie galactique consiste à disséquer et analyser les nombreuses composantes de la Voie Lactée afin de mettre en évidence et distinguer les processus physiques qui contribuent à sa formation et son évolution. Ceci est possible grâce à une estimation précise des positions, des vitesses ainsi que des propriétés de l'atmosphère stellaire des étoiles individuelles qui appartiennent aux différents populations stellaires qui composent chacune de ces composantes. De ce fait, ce domaine dépend non seulement d'observations photométriques, astrométriques et spectroscopiques permettant de mesurer
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Schlawin, Everett A. "Radiative Transfer Models of the Galactic Center." Oberlin College Honors Theses / OhioLINK, 2009. http://rave.ohiolink.edu/etdc/view?acc_num=oberlin1249300204.

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Hawkins, Keith A. "Searching for Solar-Type Hypervelocity Stars." Ohio University Honors Tutorial College / OhioLINK, 2013. http://rave.ohiolink.edu/etdc/view?acc_num=ouhonors1367583430.

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García, Pérez Ana E., Carlos Allende Prieto, Jon A. Holtzman, et al. "ASPCAP: THE APOGEE STELLAR PARAMETER AND CHEMICAL ABUNDANCES PIPELINE." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621372.

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The Apache Point Observatory Galactic Evolution Experiment (APOGEE) has built the largest moderately high-resolution (R approximate to 22,500) spectroscopic map of the stars across the Milky Way, and including dust-obscured areas. The APOGEE Stellar Parameter and Chemical Abundances Pipeline (ASPCAP) is the software developed for the automated analysis of these spectra. ASPCAP determines atmospheric parameters and chemical abundances from observed spectra by comparing observed spectra to libraries of theoretical spectra, using. 2 minimization in a multidimensional parameter space. The package
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Books on the topic "Galaxy: centre"

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N, Epchtein, ed. Science with astronomical near-infrared sky surveys: Proceedings of the Les Houches School, Centre de physique des Houches, Les Houches, France, 20-24 September, 1993. Kluwer Academic Publishers, 1994.

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International Conference 'Toward a New Millennium in Galaxy Morphology: from z=0 to the Lyman Break (1999 Midrand, South Africa). Toward a new millennium in galaxy morphology: Proceedings of an International Conference 'Toward a New Millennium in Galaxy Morphology: from z=0 to the Lyman Break, held at the Eskom Conference Centre, Midrand, South Africa, September 13-18, 1999. Kluwer Academic Publishers, 2000.

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Morris, Mark, ed. The Center of the Galaxy. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2362-1.

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Harrell, Sara Gordon. From the girls in the galaxy: Journeys to the center of ourselves. New Chapter Press, 1990.

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Joel, Davis. Journey to the center of our galaxy: A voyage in space and time. Contemporary Books, 1991.

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Bahcall, John N. PKS 2349-014: A luminous quasar with thin wisps, a large off-center nebulosity, and a close companion galaxy. National Aeronautics and Space Administration, 1995.

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Sofia, Kirhakos, Schneider Donald P, and United States. National Aeronautics and Space Administration., eds. PKS 2349-014: A luminous quasar with thin wisps, a large off-center nebulosity, and a close companion galaxy. National Aeronautics and Space Administration, 1995.

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Sofia, Kirhakos, Schneider Donald P, and United States. National Aeronautics and Space Administration., eds. PKS 2349-014: A luminous quasar with thin wisps, a large off-center nebulosity, and a close companion galaxy. National Aeronautics and Space Administration, 1995.

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Sofia, Kirhakos, Schneider Donald P, and United States. National Aeronautics and Space Administration., eds. PKS 2349-014: A luminous quasar with thin wisps, a large off-center nebulosity, and a close companion galaxy. National Aeronautics and Space Administration, 1995.

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Galactic, Center Workshop (1998 Tucson Ariz ). The central parsecs of the Galaxy: Galactic center workshop : proceedings of a meeting held at Tucson, Arizona, USA 7-11 September, 1998. Astronomical Society of the Pacific, 1999.

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Book chapters on the topic "Galaxy: centre"

1

Boyce, P. J., and R. J. Cohen. "OH in the Galactic Centre." In The Center of the Galaxy. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2362-1_16.

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van Gorkom, J. H., U. J. Schwarz, and J. D. Bregman. "Recombination-Line Observations of the Galactic Centre." In The Milky Way Galaxy. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5291-1_75.

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Seiradakis, J. H., W. Reich, and Y. Sofue. "Symmetrical Structures in the Galactic Centre Region." In The Center of the Galaxy. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2362-1_31.

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Allen, D. A., A. R. Hyland, D. J. Hillier, and J. A. Bailey. "The Stars that Power the Galactic Centre." In The Center of the Galaxy. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2362-1_72.

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Skinner, G. K. "X-Ray Observations of the Galactic Centre." In The Center of the Galaxy. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2362-1_80.

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Rees, Martin J. "Phenomena at the Galactic Centre — A Massive Black Hole?" In The Milky Way Galaxy. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5291-1_77.

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Cohen, R. J., M. Shepherd, M. J. Gaylard, and M. E. West. "OH-IR Sources and the Galactic Centre Distance." In The Center of the Galaxy. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2362-1_5.

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Pudritz, Ralph E. "Gas Dynamics in the Galactic Centre: Gravity vs. Magnetism." In The Center of the Galaxy. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2362-1_44.

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Lasenby, J., A. N. Lasenby, and F. Yusef-Zadeh. "HI Absorption Measurements over the Galactic Centre Radio Arc and Arches Regions." In The Center of the Galaxy. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2362-1_38.

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Lindqvist, M., A. Winnberg, H. J. Habing, H. E. Matthews, and F. M. Olnon. "The Mass Distribution in the Galactic Centre Estimated from OH/IR stars." In The Center of the Galaxy. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2362-1_70.

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Conference papers on the topic "Galaxy: centre"

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Ibbett, David. "Composing Music from Black Hole AGN Spectra." In ICAD 2024: The 29th International Conference on Auditory Display. International Community for Auditory Display, 2024. http://dx.doi.org/10.21785/icad2024.015.

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Black Hole Symphony is an audiovisual symphony touring planetariums and science centers across the US, with the goal of communicating the richness of science to a wide audience. Composed in 5 movements, the composition is derived from a single harmonic structure: a sonification of the electromagnetic emissions from a black hole's Active Galactic Nucleus (AGN). Originating from a complex 3- dimensional structure of dust and gas, these emissions span the entire electromagnetic spectrum - a range of &gt;20 orders of magnitude or 60 octaves - and thus far exceed the frequency span of our eyes. In
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Rampadarath, Hayden, Michael Garrett, Tom W. B. Muxlow, Gyula Jozsa, Tom Oosterloo, and Zsolt Paragi. "Is an obscured AGN at the centre of the disk galaxy IC 2497 responsible for Hanny's Voorwerp?" In The 8th International e-VLBI Workshop. Sissa Medialab, 2009. http://dx.doi.org/10.22323/1.082.0009.

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Morris, Mark. "The central engine and activity at the galactic center." In Back to the Galaxy. AIP, 1992. http://dx.doi.org/10.1063/1.44027.

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H. AZEEZ, Jazeel. "STUDYING SOME PHYSICAL PROPERTIES OF NGC 34 IN THE SUBMILLIMETER AND INFRARED WAVELENGTHS." In VI.International Scientific Congress of Pure,Applied and Technological Sciences. Rimar Academy, 2022. http://dx.doi.org/10.47832/minarcongress6-11.

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Understanding the galaxy's center few hundred parsecs is important for knowing how galaxies form and evolve. Since molecular gas is the source of star formation, it is an essential part of the interstellar medium (ISM). In this work, we display highresolution data from the Atacama Large Millimeter/Sub-millimeter Array (ALMA) of 12CO(J = 6 - 5) emission line toward the center of the galaxy NGC 34 at the distance of 85.2 Mpc (1 arcsec = 412 pc). The center area of this galaxy has drawn in the CO emission line with a resolution of (0.27ʺ × 0.23ʺ) as viewed by ALMA along with Spitzer 24 µm data. T
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Ventura, Sofia. "Untangling the Complexity in the Galactic Centre: a way to understand the origin of the gamma-ray emission from the inner Galaxy." In 37th International Cosmic Ray Conference. Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0901.

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Lis, D. C., and J. E. Carlstrom. "Dust emission in the Galactic center." In Back to the Galaxy. AIP, 1992. http://dx.doi.org/10.1063/1.43931.

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Rieke, Marcia J. "Stellar populations at the galactic center." In Back to the Galaxy. AIP, 1992. http://dx.doi.org/10.1063/1.43954.

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Kopylova, F., and A. Kopylov. "Study of groups/clusters of galaxies with the SDSS." 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/vak2021.2022.1.1.148.

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For a large sample of groups/clusters of galaxies (N =185), we obtained the scaling relations among of their photometricaland dynamical parameters. We find:0.77±0.011. that in the virialized regions of the galaxy systems the total luminosity increase with mass L K ∝ M 200(M K &lt;−21. m 0);2. that the new halo boundary of the galaxy systems corresponds to the splashback radius R sp . These radius is definedby the observed intergrated distribution of the number of galaxies as a function of the angular distance from thegroup/cluster center squared;3. that the fraction of galaxies with quenched sta
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Marr, J. M., C. Lemme, T. A. Pauls, M. C. H. Wright, T. L. Wilson, and A. L. Rudolph. "High resolution study of the −190 km s−1 molecular gas in the Galactic center; IRAM observations of CO J=1→0 and J=2→1 in the central 80‘." In Back to the Galaxy. AIP, 1992. http://dx.doi.org/10.1063/1.43971.

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Ozernoy, L. M. "Evaluating the mass of a putative black hole at the Galactic center." In Back to the Galaxy. AIP, 1992. http://dx.doi.org/10.1063/1.43951.

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Reports on the topic "Galaxy: centre"

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Moran, Lisa, Sheila Garrity, Caroline McGregor, and Carmel Devaney. Hoping for a Better Tomorrow: A Process Study Evaluation of the Greater Tomorrow Creche and Ballyhaunis Community Preschool Services, Ballyhaunis, Co. Clare. Institute for Lifecourse and Society National University of Ireland, Galway, 2016. http://dx.doi.org/10.52516/plpu6954.

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This report presents the results of a qualitative, process study evaluation of the Ballyhaunis Community Preschool and ‘Greater Tomorrow’ crèche services, conducted by the UNESCO Child and Family Research Centre (UCFRC), NUI, Galway in 2015.
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Tierney, Edel, Cormac Forkan, Bernadine Brady, and Rebecca Jackson. Tusla’s Programme for Prevention, Partnership and Family Support:Children’s Participation Work Package : Final Report. University of Galway, 2018. http://dx.doi.org/10.52516/tkii4235.

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The Development and Mainstreaming Programme for Prevention, Partnership and Family Support (PPFS) is a programme of action being undertaken by Tusla, the Child and Family Agency, as part of its National Service Delivery Framework. The programme seeks to embed prevention and early intervention into the culture and operation of Tusla. The UNESCO Child and Family Research Centre, NUI Galway has undertaken an evaluation study focusing on the implementation of and the outcomes from the PPFS programme. The study’s overall research question is: Is the organisational culture and practice of Tusla and
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Cassidy, Anne, Leonor Rodriguez, and Carmel Devaney. The Child and Family Support Networks Research Study. UNESCO Child and Family Research Centre, National University of Ireland Galway, 2018. http://dx.doi.org/10.52516/eaoa2611.

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The research and evaluation team at the UNESCO Child and Family Research Centre (UCFRC), NUI Galway provides research, evaluation and technical support to Tusla’s Development and Mainstreaming Programme for Prevention, Partnership and Family Support (PPFS). This is a new programme of action being undertaken by Tulsa – Child and Family Agency as part of its National Service Delivery Framework. The programme seeks to transform child and family services in Ireland by embedding prevention and early intervention into the culture and operations of Tusla. The research and evaluation carried out by th
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