Search Results - "Centaurus"

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    Thermal plasma in the giant lobes of the radio galaxy Centaurus A by O'Sullivan, S., Feain, I., McClure-Griffiths, N., Ekers, Ronald, Carretti, E., Robishaw, T., Mao, S., Gaensler, B., Bland-Hawthorn, J., Stawarz

    Published 2013
    “…We present a Faraday rotation measure (RM) study of the diffuse, polarized, radio emission from the giant lobes of the nearest radio galaxy, Centaurus A. After removal of the smooth Galactic foreground RM component, using an ensemble of background source RMs located outside the giant lobes, we are left with a residual RM signal associated with the giant lobes. …”
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    HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster by Fabian, A.C., Walker, S.A., Russell, H.R., Pinto, C., Canning, R.E.A., Salome, P., Sanders, J.S., Taylor, G.B., Zweibel, E.G., Conselice, Christopher J., Combes, F., Crawford, C.S., Ferland, G.J., Gallager, J.S., Hatch, Nina A., Johnstone, R.M., Reynolds, C.S.

    Published 2016
    “…Narrow-band HST imaging has resolved the detailed internal structure of the 10 kpc diameter H α+[N II] emission line nebulosity in NGC4696, the central galaxy in the nearby Centaurus cluster, showing that the dusty, molecular, filaments have a width of about 60 pc. …”
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    On the magnetic field through the Upper Centaurus-Lupus super bubble in the vicinity of the Southern Coalsack by Bhat, Ramesh, Andersson, B.

    Published 2011
    “…The Southern Coalsack is located in the interior of the Upper Centaurus-Lupus (UCL) super bubble and shows many traits that point to a much more energetic environment than might be expected from a dark, starless molecular cloud. …”
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    Discovery of Very High Energy gamma-Ray Emission from Centaurus a with H.E.S.S. by Aharonian, F., Akhperjanian, A., Anton, G., De Almeida, U., Bazer-Bachi, A., Becherini, Y., Behera, B., Benbow, W., Bernlöhr, K., Boisson, C., Bochow, A., Borrel, V., Brion, E., Brucker, J., Brun, P., BüHLER, R., Bulik, T., Büsching, I., Boutelier, T., Chadwick, P., Charbonnier, A., Chaves, R., Cheesebrough, A., Chounet, L., Clapson, A., Coignet, G., Dalton, M., Daniel, M., Davids, I., Degrange, B., Deil, C., Dickinson, H., Djannati-Ataï, A., Domainko, W., Drury, L., Dubois, F., Dubus, G., Dyks, J., Dyrda, M., Egberts, K., Emmanoulopoulos, D., Espigat, P., Farnier, C., Feinstein, F., Fiasson, A., Förster, A., Fontaine, G., Füling, M., Gabici, S., Gallant, Y., Gerard, L., Giebels, B., Glicenstein, J., Glück, B., Goret, P., Göhring, D., Häuser, D., Hauser, M., Heinz, S., Heinzelmann, G., Henri, G., Hermann, G., Hinton, J., Hoffmann, A., Hofmann, W., Holleran, M., Hoppe, P., Horns, D., Jacholkowska, A., De Jager, O., Jahn, C., Jung, I., Katarzynski, K., Katz, U., Kaufmann, S., Kendziorra, E., Kerschhaggl, M., Khangulyan, D., Khélifi, B., Keogh, D., Kluzniak, W., Kneiske, T., Komin, N., Kosack, K., Lamanna, G., Latham, I., Lenain, J., Lohse, T., Marandon, V., Martin, J., Martineau-Huynh, O., Marcowith, A., Maurin, D., McComb, T., Medina, C., Moderski, R., Moulin, E., Naumann-Godo, M., de Naurois, M., Nedbal, D., Nekrassov, D., Niemiec, J., Nolan, S., Ohm, S., Olive, J., de Oña Wilhelmi, E., Orford, K., Ostrowski, M., Panter, M., Paz Arribas, M., Pedaletti, G., Pelletier, G., Petrucci, P., Pita, S., Pühlhofer, G., Punch, M., Quirrenbach, A., Raubenheimer, B., Raue, M., Rayner, S., Renaud, M., Rieger, F., Ripken, J., Rob, L., Rosier Lees, S., Rowell, G., Rudak, B., Rulten, C., Ruppel, J., Sahakian, V., Santangelo, A., Schlickeiser, R., Schöck, F., Schröder, R., Schwanke, U., Schwarzburg, S., Schwemmer, S., Shalchi, A., Sikora, M., Skilton, J., Sol, H., Spangler, D., Stawarz, L., Steenkamp, R., Stegmann, C., Superina, G., Szostek, A., Tam, P., Tavernet, J., Terrier, R., Tibolla, Omar, Tluczykont, M., van Eldik, C., Vasileiadis, G., Venter, C., Venter, L., Vialle, J., Vincent, P., Vink, J., Vivier, M., Volk, H., Volpe, F., Wagner, S., Ward, M., Zdziarski, A., Zech, A.

    Published 2009
    “…Centaurus A has been observed for more than 120 hr. …”
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    Filaments in the southern giant lobe of Centaurus A: Constraints on nature and origin from modelling and GMRT observations by Wykes, S., Intema, Hubertus, Hardcastle, M., Achterberg, A., Jones, T., Jerjen, H., Orrú, E., Lazarian, A., Shimwell, T., Wise, M., Kronberg, P.

    Published 2014
    “…We present results from imaging of the radio filaments in the southern giant lobe of CentaurusA using data from Giant Metrewave Radio Telescope observations at 325 and 235 MHz, and outcomes from filament modelling. …”
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    Is there a giant Kelvin-Helmholtz instability in the sloshing cold front of the Perseus cluster? by Walker, S., Hlavacek-Larrondo, J., Gendron-Marsolais, M., Fabian, A., Intema, Hubertus, Sanders, J., Bamford, J., van Weeren, R.

    Published 2017
    “…Deep observations of nearby galaxy clusters with Chandra have revealed concave ‘bay’ structures in a number of systems (Perseus, Centaurus and Abell 1795), which have similar X-ray and radio properties. …”
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    Status report and future prospects on LUNASKA lunar observations with ATCA by James, C., Ekers, Ronald, Alvarez-Muñiz, J., Protheroe, R., McFadden, R., Phillips, C., Roberts, P.

    Published 2009
    “…We have observed so as to maximise the UHE neutrino sensitivity in the region surrounding the galactic centre and to Centaurus A, to which current limits on the highest-energy neutrinos are relatively weak. …”
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    Status and strategies of current LUNASKA lunar Cherenkov observations with the Parkes radio telescope by Bray, J., Ekers, Ronald, Roberts, P., Reynolds, J., James, C., Phillips, C., McFadden, R., Protheroe, R., Aartsen, M., Alvarez-Muniz, J.

    Published 2012
    “…We also briefly describe the flux limits which we expect to set with our current observations, including a directional limit for Centaurus A.…”
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    Limit on the ultrahigh-energy neutrino flux from lunar observations with the Parkes radio telescope by Bray, J., Ekers, Ronald, Roberts, P., Reynolds, J., James, C., Phillips, C., Protheroe, R., McFadden, R., Aartsen, M.

    Published 2015
    “…The targeting strategy of the observations also allows us to place a directional limit on the neutrino flux from the nearby radio galaxy Centaurus A.…”
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    The kinematics and orbital dynamics of the PSR B1259-63/LS 2883 system from 23 yr of pulsar timing by Shannon, Ryan, Johnston, S., Manchester, R.

    Published 2014
    “…We also measure a significant proper motion that locates the birth of the system in the Centaurus OB1 association. By combining proper motion of the pulsar with radial velocity measurements of the companion, we measure the three-dimensional velocity of the system. …”
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