Relevant bibliographies by topics / Galaxies – Spectres

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

Academic literature on the topic 'Galaxies – Spectres'

Author: Grafiati
Published: 4 June 2021
Last updated: 8 February 2022

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Journal articles on the topic "Galaxies – Spectres"

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Reynolds, T. N., T. Westmeier, and L. Staveley-Smith. "H i deficiencies and asymmetries in HIPASS galaxies." Monthly Notices of the Royal Astronomical Society 499, no. 3 (2020): 3233–42. http://dx.doi.org/10.1093/mnras/staa3126.

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ABSTRACT We present an analysis of the sky distribution of neutral hydrogen (H i) deficiency and spectral asymmetry for galaxies detected by the H i Parkes All-Sky Survey (HIPASS) as a function of projected environment density. Previous studies of galaxy H i deficiency using HIPASS were sensitive to galaxies that are extremely H i rich or poor. We use an updated binning statistic for measuring the global sky distribution of H i deficiency that is sensitive to the average deficiencies. Our analysis confirms the result from previous studies that galaxies residing in denser environments, such as
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Delgado, Rosa González, Enrique Pérez, Roberto Cid Fernandes, et al. "CALIFA survey: The spatially resolved star formation history of massive galaxies." Proceedings of the International Astronomical Union 8, S295 (2012): 300–303. http://dx.doi.org/10.1017/s1743921313005097.

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AbstractThe Calar Alto Legacy Integral Field Area (CALIFA) project is an ongoing 3D spectroscopic survey of 600 nearby galaxies of all kinds. This pioneer survey is providing valuable clues on how galaxies form and evolve. Processed through spectral synthesis techniques, CALIFA datacubes allow us to, for the first time, spatially resolve the star formation history of galaxies spread across the color-magnitude diagram. The richness of this approach is already evident from the results obtained for the first ~ 1/6 of the sample. Here we show how the different galactic spatial sub-components (“bul
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González Delgado, R. M., E. Pérez, R. Cid Fernandes, et al. "The growth of mass and metallicity in bulges and disks: CALIFA perspective." Proceedings of the International Astronomical Union 10, H16 (2012): 338. http://dx.doi.org/10.1017/s1743921314006024.

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AbstractCALIFA (Calar Alto Legacy Integral Field Area) is a 3D spectroscopic survey of 600 nearby galaxies that we are obtaining with PPaK@3.5m at Calar Alto (Sánchez et al. 2012; Husemann et al. 2012). This pioneer survey is providing valuable clues on how the mass and metallicity grow in the different galactic spatial sub-components (“bulge” and “disk”). Processed through spectral synthesis techniques, CALIFA datacubes allow us to, for the first time, spatially resolve the star formation history of galaxies (Cid Fernandes et al. 2012). The richness of this approach is already evident from th
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Franco, M., D. Elbaz, L. Zhou, et al. "GOODS-ALMA: The slow downfall of star formation in z = 2–3 massive galaxies." Astronomy & Astrophysics 643 (October 27, 2020): A30. http://dx.doi.org/10.1051/0004-6361/202038312.

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We investigate the properties of a sample of 35 galaxies, detected with the Atacama Large Millimeter/Submillimeter Array (ALMA) at 1.1 mm in the GOODS-ALMA field (area of 69 arcmin2, resolution = 0.60″, rms ≃ 0.18 mJy beam−1). Using the ultraviolet-to-radio deep multiwavelength coverage of the GOODS–South field, we fit the spectral energy distributions of these galaxies to derive their key physical properties. The galaxies detected by ALMA are among the most massive at z = 2−4 (M⋆, med = 8.5 × 1010 M⊙) and they are either starburst or located in the upper part of the galaxy star-forming main s
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Briggs, F. H. "VLBI Studies of High-Redshift 21cm Absorption Lines." Symposium - International Astronomical Union 129 (1988): 211. http://dx.doi.org/10.1017/s0074180900134503.

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VLBI experiments can contribute to our understanding of absorbing gas observed in the spectra of high-redshift quasars by measuring the spatial extent of the absorbers. An optical survey conducted by Wolfe, Turnshek, Smith, and Cohen (1986) has turned up a class of absorbers characterized by large HI column density and a rich spectrum of metal absorption lines. In these respects the absorbers resemble spiral galaxies, but their occurence is too frequent for interception probabilities based on galaxy cross sections at the present epoch. Recent radio observations to determine the nature of such
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Andreasian-Thomas, Nora. "Dusty Active Galaxies." Proceedings of the International Astronomical Union 9, S304 (2013): 65. http://dx.doi.org/10.1017/s1743921314003330.

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AbstractMost astronomers know about B. E. Markarians discovery and further study of galaxies with UV excess. It is less known that in 1963 Markarian drew attention to a small group of galaxies with color index-spectral type discrepancy. Early spectral type of these galaxies is combined with large color index (e.g. M82). Later studies showed that galaxies with large intrinsic color indices (CI ≥ 0.85) exhibit properties typical for active galaxies - galaxies with “red excess” are as active as galaxies with UV excess.
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Sodré, L., and H. Cuevas. "Spectral classification of galaxies." Vistas in Astronomy 38 (January 1994): 287–91. http://dx.doi.org/10.1016/0083-6656(94)90039-6.

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Jackson, C. A., and D. M. Londish. "Spectral Characteristics of the 2dFGRS–NVSS Galaxies." Publications of the Astronomical Society of Australia 17, no. 3 (2000): 234–40. http://dx.doi.org/10.1071/as00042.

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AbstractWe have analysed the 2dF spectra of a sample of galaxies common to the 2dF Galaxy Redshift Survey (2dFGRS, Colless 1999) and the NRAO VLA Sky Survey (NVSS, Condon et al. 1998). Our sample comprises 88 galaxies selected by Sadler et al. (1999) from 30 2dFGRS fields observed in 1998. In this paper we discuss how this and future, much larger, samples of 2dFGRS–NVSS galaxies can be interpreted via analysis of those galaxies with strong narrow emission lines. Using diagnostic line ratio measurements, we confirm the majority of the eyeball classifications of Sadler et al. (1999), although ma
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Denissyuk, E. K., V. N. Gaisina, and R. R. Valiullin. "Spectral Variability of Some Seyfert Galaxies." International Astronomical Union Colloquium 184 (2002): 361–62. http://dx.doi.org/10.1017/s0252921100031031.

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AbstractThe very first spectrograms of 40 Seyfert galaxies are discussed. All these objects were taken from Markarian’s lists of galaxies. They were first investigated and classified at Fesenkov Astrophysical Institute during 1973-1988. Spectral study was carried out with a slit spectrograph, attached to the 70-cm telescope and equipped with a three cascades image-tube. Repeated observations of 22 galaxies were obtained in 1985-2000. An analysis of possible spectral variability of the studied galaxies over 10-26 years was made. A list of objects which are the most interesting for further obser
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Feltre, Anna, Evanthia Hatziminaoglou, Antonio Hernán-Caballero, Jacopo Fritz, and Alberto Franceschini. "AGN and Star Formation in HerMES-IRS sources." Proceedings of the International Astronomical Union 9, S304 (2013): 52–55. http://dx.doi.org/10.1017/s1743921314003305.

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AbstractOne of the remaining open issues in the context of the analysis of Active Galactic Nuclei (AGN) is the evidence that nuclear gravitational accretion is often accompanied by a concurrent starburst activity. We developed a spectral energy distribution (SED) fitting technique to derive simultaneously the physical properties of active galaxies and coexisting starbursts making the best use of Spitzer and Herschel IR observations. We apply the SED fitting procedure to a large sample of extragalactic sources representing the HerMES (Herschel/Multi-tiered Extragalactic Survey) population with
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Dissertations / Theses on the topic "Galaxies – Spectres"

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Fremaux, Julien. "Populations stellaires dans les galaxies hôtes de noyaux actifs." Paris 7, 2006. http://www.theses.fr/2006PA077102.

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La population stellaire des galaxies hôtes de noyau actif semble entretenir une relation étroite avec le degré d'activité du noyau. Ces galaxies étant trop éloignées pour qu'il soit possible de les résoudre en étoiles individuelles, il faut faire appel à une méthode de synthèse de population pour déterminer quels types d'étoiles les composent. La comparaison de ces populations stellaires avec celles de galaxies non-actives de même type morphologique nous permettra d'en savoir plus sur l'interaction entre la population stellaire et le noyau actif. Dans cette thèse, nous avons développé une nouv
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Maffei, Bruno. "Etude des galaxies dans le domaine submillimétrique et réalisation d'un spectromètre refroidi." Paris 7, 1994. http://www.theses.fr/1994PA077269.

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Les observations faites par le satellite iras dans l'infrarouge lointain ont révélé l'importance de ce domaine spectral dans l'étude des galaxies et en particulier celles de type Starburst. Il est discuté dans cette thèse de la possibilité de détection des galaxies par les prochaines générations d'instruments dans les domaines infrarouge lointain et submillimétrique. Pour cela une modélisation du spectre des galaxies incluant le continuum et les raies d'émission des PAH (molécules polycycliques aromatiques hydrocarbonées) a été effectuée ainsi qu'un modèle logarithme n - logarithme s donnant u
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Roman, Matthieu. "Amas de galaxies détectés par Planck avec l'effet Sunyaev-Zel'dovich thermique : contraintes cosmologiques et spectre angulaire." Paris 7, 2014. http://www.theses.fr/2014PA077099.

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L'un des enjeux de la cosmologie moderne dans le cadre du modèle standard régi par la relativité générale est de déterminer la nature de l'énergie noire et de caractériser le comportement et l'évolution de la matière ordinaire piégée dans les puits de potentiel de la matière noire. Les amas de galaxies, en tant que traceurs uniques de l'évolution des structures, sont particulièrement adaptés pour remplir ces conditions. Grâce à l'effet Sunyaev-Zel'dovich (SZ) thermique, nom donné à l'interaction Compton inverse entre les photons du fond diffus cosmologique et le gaz dense d'électrons au sein d
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Gonçalves, Anabela Cardoso. "Etude spectroscopique des noyaux actifs de galaxies à "spectre de transition"." Aix-Marseille 1, 1999. http://www.theses.fr/1999AIX11081.

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Les noyaux de galaxies présentent souvent des raies en émission ; ils sont classés en plusieurs catégories sur la base des rapports d'intensité de quelques raies dans le visible : Seyferts 1 et 2, LINERs et régions HII ; ces catégories correspondent à des conditions d'excitations différentes. Mais un certain nombre d'objets ont des rapports de raies intermédiaires qui ne permettent pas de les classer sans ambiguité dans l'une ou l'autre de ces catégories. Nous nous sommes efforcés de clarifier la nature de ces objets à "spectre de transition". Pour ce faire, nous avons effectué des observation
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Torres, Flores Sergio Patricio. "Etude de la cinématique des galaxies dans les groupes compacts." Aix-Marseille 1, 2010. http://theses.univ-amu.fr.lama.univ-amu.fr/2010AIX11050.pdf.

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Cette thèse présente les résultats concernant la structure, les relations d'échelle et la cinématique de 48 galaxies au sein de 22 groupes compacts de Hickson, sachant que pour 35 d'entre elles au sein de 12 groupes, ce travail présente des cartes monochromatiques, de vitesses et de dispersion de vitesses originales pour la ligne H. Les différents paramètres cinématiques et les courbes de rotation ont été déduits de ces cartes de vitesses ainsi que d'images dans le domaine optique. En utilisant les vitesses maximales de rotation (déduites des courbes de rotation), les luminosités tant dans le
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Poncelet, Anne. "Etude de l'émission infrarouge au coeur des noyaux actifs de galaxies : le cas de NGC 1068." Paris 7, 2007. http://www.theses.fr/2007PA077203.

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CETTE THESE EST CONSACREE A L'ETUDE DES NOYAUX ACTIFS DE GALAXIES (NAG) EN INFRAROUGE. ELLE PORTE PLUS PARTICULIEREMENT SUR LA POUSSIÈRE - ÉLÉMENT CLÉ DU SCHÉMA UNIFIÉ DES NAGS - DISTRIBUÉE AU COEUR DE NGC 1068, OBSERVÉE AVEC DES INSTRUMENTS DU VERY LARGE TELESCOPE DE L'ESO (OBSERVATOIRE EUROPÉEN AUSTRAL). L'INTERFÉROMÈTRE MIDI RÉSOUD LA POUSSIÈRE DE NGC 1068 À DE TRÈS PETITES ÉCHELLES (<br>This thesis is devoted to the study of active galactic nuclei (agn) in the infrared band. It is particularly based on the dust - key component of the unified scheme of agns - distributed in the cori of ngc
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Burgarella, Denis. "Automatisation du traitement de spectres bidimensionnels a l'aide d'algorithmes de reconnaissance de formes : application a des spectres de galaxies (mkn 171) et d'etoiles sous-naines." Nice, 1987. http://www.theses.fr/1987NICE4161.

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Traitement des spectres de moyenne dispersion obtenus avec des spectrographes a longue fente equipes d'un tube image a 2 dimensions. Un algorithme de reconnaissance de formes permet de traiter et corriger geometriquement les donnees sans se preoccuper de leur origine. L'application a des objets etendus (galaxies) et compacts (etoiles) sert de test pour ce nouveau traitement spectral automatique. Une etoile sous naine (cpd-71 **(o) 172) observee par le satellite iue en uv est etudiee en detail
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Plat, Adèle. "Modélisation et interprétation des propriétés spectrales des galaxies primordiales." Thesis, Sorbonne université, 2019. http://www.theses.fr/2019SORUS298.

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Pendant le premier milliard d’années de l’Univers, les premières galaxies se sont formées et ont réionisé le milieu intergalactique. Grâce au James Webb Space Telescope, l’observation de spectres ultraviolets et optiques des galaxies de l’époque de la réionisation sera bientôt possible. L’émission de ces galaxies contient des informations précieuses sur leurs propriétés physiques et en particulier sur la caractérisation des sources à l’origine de la réionisation de l’Univers. Nous explorons des modèles physiquement auto consistants de galaxies à formation d’étoiles, en incluant l’émission du g
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Lecureur, Aurélie. "Contraintes observationnelles sur la formation et l’évolution chimique du bulbe galactique." Observatoire de Paris (1667-....), 2007. https://hal.science/tel-02071421.

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Le bulbe de la Voie Lactée présente des caractéristiques contradictoires. D'une part sa morphologie est proche de celles des galaxies tardives barrées, dont la formation est reliée aux instabilités du disque ("pseudo-bulbe"). D'autre part, il semble constitué de populations stellaires vieilles et métalliques qui évoque les sphéroïdes des galaxies précoces (bulbes classiques). C'est dans ce contexte que se place le travail de cette thèse. Profitant de l'installation de l'instrument FLAMES au VLT, nous avons observé 5 échantillons d'environ 230 étoiles géantes du bulbe dans des champs distribués
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Zou, Siwei. "Using quasar absorption lines to probe cold gas in high redshift galaxies." Thesis, Sorbonne université, 2018. http://www.theses.fr/2018SORUS181/document.

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Les raies d'absorption de quasars sont des outils efficaces pour étudier le milieu interstellaire dans les galaxies. Dans ce travail, nous étudions un échantillon de soixante-six systèmes absorbants à z&lt;1.5 sélectionnés pour la présence de raies d'absorption de CI intenses dans leurs spectres SDSS. Ils sont observés par les spectrographes X-shooter et UVES du VLT de l'ESO. Nous étudions en tout 17 systèmes observés par X-shooter. Nous déduisons la métallicité, la déplétion par la poussière, le taux d'extinction par la poussière et le taux d'absorption des raies de MgII, MgI, CaII et NaI déc
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Books on the topic "Galaxies – Spectres"

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Chiosi, Cesare, and Alvio Renzini, eds. Spectral Evolution of Galaxies. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4598-2.

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Stein, W. A. Spectral components at visual and infrared wavelengths in active galactic nuclei. University of Hawaii, Institute for Astronomy, 1985.

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Colloquium, International Astronomical Union. Probing galaxies through quasar absorption lines: Proceedings of the 199th colloquium of the International Astronomical Union held in Shanghai, People's Republic of China, March 14-18, 2005. Cambridge University Press, 2005.

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SED, 2004 (2004 Heidelberg Germany). The spectral energy distributions of gas-rich galaxies: Confronting models with data : international workshop, Heidelberg, Germany, 4-8 October 2004 : SED 2004 Heidelberg. American Institute of Physics, 2005.

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David, Moore. Spectra of high-ionization Seyfert 1 galaxies: Implications for the narrow-line region. National Aeronautics and Space Administration, 1997.

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Brahic, A. Lumières d'étoiles: Les couleurs de l'invisible. Jacob, 2008.

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Huchtmeier, W. K. A general catalog of HI observations of galaxies: The reference catalog. Springer-Verlag, 1989.

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Chris, Blades J., Turnshek David Alvin, Norman Colin A, and Space Telescope Science Institute (U.S.), eds. QSO absorption lines: Probing the universe : proceedings of the QSO Absorption Line Meeting, Baltimore, 1987, May 19-21. Cambridge University Press, 1988.

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Turner, T. J. PSPC soft x-ray observations of Seyfert 2 galaxies. High Energy Astrophysics Science Archive Research Center, NASA Goddard Space Flight Center, 1993.

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Turner, T. J. PSPC soft X-ray observations of Seyfert 2 galaxies. High Energy Astrophysics Science Archive Research Center, NASA Goddard Space Flight Center, 1993.

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Book chapters on the topic "Galaxies – Spectres"

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Bond, J. Richard. "Testing Cosmic Fluctuation Spectra." In Nearly Normal Galaxies. Springer New York, 1987. http://dx.doi.org/10.1007/978-1-4612-4762-3_44.

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Rocca-Volmerange, B., and B. Guiderdoni. "Spectral Evolution of Galaxies." In The World of Galaxies. Springer US, 1989. http://dx.doi.org/10.1007/978-1-4613-9356-6_79.

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Bruzual, Gustavo A. "Spectral Evolution of Galaxies." In Spectral Evolution of Galaxies. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4598-2_21.

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Lauger, S., D. Burgarella, and V. Buat. "Spectro-Morphology of Galaxies." In The Evolution of Galaxies. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-3315-1_135.

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Lauger, Sebastien, Denis Burgarella, and Veronique Buat. "Spectro-Morphology of Galaxies." In Multiwavelength Cosmology. Springer Netherlands, 2004. http://dx.doi.org/10.1007/0-306-48570-2_16.

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de Jong, Teije. "Galaxies in the Infrared." In Spectral Evolution of Galaxies. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4598-2_12.

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Barbaro, G., and F. M. Olivi. "Spectrophotometric Models of Galaxies." In Spectral Evolution of Galaxies. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4598-2_22.

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Terlevich, Roberto. "AGN as Starbursts: modelling the multifrequency spectrum." In Windows on Galaxies. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0543-6_12.

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Silk, Joseph. "Galaxy Evolution: Some Issues and Questions." In Spectral Evolution of Galaxies. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4598-2_1.

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Madore, Barry F. "Galaxy Encounters and the Holmberg Effect." In Spectral Evolution of Galaxies. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4598-2_10.

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Conference papers on the topic "Galaxies – Spectres"

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Lisitsin, D. D., and A. V. Kuzin. "Identification of extragalactic star forming complexes." In Всероссийская с международным участием научная конференция студентов и молодых ученых, посвященная памяти Полины Евгеньевны Захаровой «Астрономия и исследование космического пространства». Ural University Press, 2021. http://dx.doi.org/10.15826/b978-5-7996-3229-8.08.

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We developed a technique for selecting star forming complexes in external galaxies based on an analysis of radiation maps in various spectral bands. Using this method, we identified star formation complex candidates in 17 nearby galaxies applying three criteria. These criteria are polycyclic aromatic hydrocarbon emission, dust emission, and ultraviolet young star emission. Relating the information derived from these criteria, we made a sample of star forming regions suitable for revealing correlations between various star formation tracers.
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Takagi, T. "Silicate-break galaxies." In THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP, 2005. http://dx.doi.org/10.1063/1.1913947.

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Brandt, W. N. "Grating X-ray Spectroscopy of High-Velocity Outflows from Active Galaxies." In SPECTRAL LINE SHAPES. AIP, 2002. http://dx.doi.org/10.1063/1.1525444.

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Townes, Charles H. "Far infrared spectra of galaxies." In International Conference on Millimeter and Submillimeter Waves and Applications 1994. SPIE, 1994. http://dx.doi.org/10.1117/12.2303020.

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Townes, Charles H., and Norbert Geis. "Far-infrared spectra of galaxies." In Millimeter and Submillimeter Waves and Applications: International Conference, edited by Mohammed N. Afsar. SPIE, 1994. http://dx.doi.org/10.1117/12.182988.

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Kylafis, Nikolaos D. "Radiation Transfer Models in Galaxies." In THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP, 2005. http://dx.doi.org/10.1063/1.1913911.

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Panuzzo, Pasquale. "Panchromatic models of galaxies: GRASIL." In THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP, 2005. http://dx.doi.org/10.1063/1.1913929.

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Arbutina, Bojan, Luka Č Popović, and Milan S. Dimitrijević. "Radial Dependence of Extinction in Parent Galaxies of Supernovae." In SPECTRAL LINE SHAPES IN ASTROPHYSICS: VI Serbi an Conference on Spectral Line Shapes in Astrophysics (VI SCSLSA). AIP, 2007. http://dx.doi.org/10.1063/1.2800129.

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Inoue, Akio K. "Attenuation law of normal disk galaxies." In THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP, 2005. http://dx.doi.org/10.1063/1.1913942.

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Jonsson, Patrik. "Simulations of Dust in Interacting Galaxies." In THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP, 2005. http://dx.doi.org/10.1063/1.1913946.

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Reports on the topic "Galaxies – Spectres"

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Mizuno, T. Accretion Disk Spectra of the Ultra-Luminous X-Ray Sources in Nearby Spiral Galaxies and Galactic Superluminal Jet Sources. Office of Scientific and Technical Information (OSTI), 2003. http://dx.doi.org/10.2172/826596.

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