Zobrazeno 1 - 10
of 62
pro vyhledávání: '"Pannuti, T. G."'
Autor:
Velović, Velibor, Filipović, M. D., Barnes, L., Norris, R. P., Tremblay, C. D., Heald, G., Rudnick, L., Shabala, S. S., Pannuti, T. G., Andernach, H., Titov, O., Waddell, S. G. H., Koribalski, B. S., Grupe, D., Jarrett, T., Alsaberi, R. Z. E., Carretti, E., Collier, J. D., Einecke, S., Galvin, T. J., Hotan, A., Manojlović, P., Marvil, J., Nandra, K., Reiprich, T. H., Rowell, G., Salvato, M., Whiting, M.
We present the discovery of highly-collimated radio jets spanning a total of 355 kpc around the nearby elliptical galaxy NGC 2663, and the possible first detection of recollimation on kiloparsec scales. The small distance to the galaxy (~28.5 Mpc) al
Externí odkaz:
http://arxiv.org/abs/2207.06713
Autor:
Filipović, M. D., Bojičić, I. S., Grieve, K. R., Norris, R. P., Tothill, N. F. H., Shobhana, D., Rudnick, L., Prandoni, I., Andernach, H., Hurley-Walker, N., Alsaberi, R. Z. E., Anderson, C. S., Collier, J. D., Crawford, E. J., For, B. -Q., Galvin, T. J., Haberl, F., Hopkins, A. M., Ingallinera, A., Kavanagh, P. J., Koribalski, B. S., Kothes, R., Leahy, D., Leverenz, H., Maggi, P., Maitra, C., Marvil, J., Pannuti, T. G., Park, L. A. F., Payne, J. L., Pennock, C. M., Riggi, S., Rowell, G., Sano, H., Sasaki, M., Staveley-Smith, L., Trigilio, V., Umana, G., Urošević, D., van Loon, J. Th., Vardoulaki, E.
We present a comprehensive multi-frequency catalogue of radio sources behind the Large Magellanic Cloud between 0.2 and 20 GHz, gathered from a combination of new and legacy radio continuum surveys. This catalogue covers an area of $\sim$144~deg$^2$
Externí odkaz:
http://arxiv.org/abs/2107.10967
Autor:
Vučetić, M. M., Ilić, D., Egorov, O. V., Moiseev, A., Onić, D., Pannuti, T. G., Arbutina, B., Petrov, N., Urošević, D.
Publikováno v:
A&A 628, A87 (2019)
In this paper we present new optical observations of the galaxy NGC 185 intended to reveal the status of supernova remnants (SNRs) in this dwarf companion of the Andromeda galaxy. Previously, it was reported that this galaxy hosts one SNR. Our deep p
Externí odkaz:
http://arxiv.org/abs/1905.02468
Autor:
Onić, D., Filipović, M. D., Bojičić, I., Hurley-Walker, N., Arbutina, B., Pannuti, T. G., Maitra, C., Urošević, D., Haberl, F., Maxted, N., Wong, G. F., Rowell, G., Bell, M. E., Callingham, J. R., Dwarakanath, K. S., For, B. -Q., Hancock, P. J., Hindson, L., Johnston-Hollitt, M., Kapińska, A. D., Lenc, E., McKinley, B., Morgan, J., Offringa, A. R., Porter, L. E., Procopio, P., Staveley-Smith, L., Wayth, R. B., Wu, C., Zheng, Q.
Publikováno v:
A&A 625, A93 (2019)
In this paper we discuss the radio continuum and X-ray properties of the so-far poorly studied Galactic supernova remnant (SNR) G5.9+3.1. We present the radio spectral energy distribution (SED) of the Galactic SNR G5.9+3.1 obtained with the Murchison
Externí odkaz:
http://arxiv.org/abs/1904.06541
Discovery of a Pulsar-powered Bow Shock Nebula in the Small Magellanic Cloud Supernova Remnant DEMS5
Autor:
Alsaberi, Rami Z. E., Maitra, C., Filipovi'c, M. D., Bozzetto, L. M., Haberl, F., Maggi, P., Sasaki, M., Manjolovi'c, P., Velovi'c, V., Kavanagh, P., Maxted, N. I., Urovsevi'c, D., Rowell, G. P., Wong, G. F., For, B. -Q., O'Brien, A. N., Galvin, T. J., Staveley-Smith, L., Norris, R. P., Jarrett, T., Kothes, R., Luken, K. J., Hurley-Walker, N., Sano, H., Oni'c, D., Dai, S., Pannuti, T. G., Tothill, N. F. H., Crawford, E. J., Yew, M., Bojivci'c, I., D'enes, H., McClure-Griffiths, N., Gurovich, S., Fukui, Y.
We report the discovery of a new Small Magellanic Cloud Pulsar Wind Nebula (PWN) at the edge of the Supernova Remnant (SNR)-DEM S5. The pulsar powered object has a cometary morphology similar to the Galactic PWN analogs PSR B1951+32 and 'the mouse'.
Externí odkaz:
http://arxiv.org/abs/1903.03226
Autor:
Maxted, Nigel I., Filipovic, M. D., Sano, H., Allen, G. E., Pannuti, T. G., Rowell, G. P., Grech, A., Roper, Q., Wong, G. F., Galvin, T. J., Fukui, Y., Collier, J. D., Crawford, E. J., Grieve, K., Horta, A. D., Manojlovic, P., O'Brien, A.
We conduct a multi-wavelength morphological study of the Galactic supernova remnant RXJ0852.0-4622 (also known as Vela Jr., Vela Z and G266.2-1.2). RX J0852.0-4622 is coincident with the edge of the larger Vela supernova remnant causing confusion in
Externí odkaz:
http://arxiv.org/abs/1809.02249
Autor:
Vucetic, M. M., Ciprijanovic, A., Pavlovic, M. Z., Pannuti, T. G., Petrov, N., Goker, U. D., Ercan, E. N.
We present the detection of 16 optical supernova remnant (SNR) candidates in the nearby spiral galaxy IC342. The candidates were detected by applying [SII]/H$\alpha$ ratio criterion on observations made with the 2 m RCC telescope at Rozhen National A
Externí odkaz:
http://arxiv.org/abs/1511.05307
Autor:
Allen, G. E., Chow, K., DeLaney, T., Filipovic, M. D., Houck, J. C., Pannuti, T. G., Stage, M. D.
An analysis of Chandra ACIS data for two relatively bright and narrow portions of the northwestern rim of G266.2-1.2 (a.k.a. RX J0852.0-4622 or Vela Jr.) reveal evidence of a radial displacement of 2.40 +/- 0.56 arcsec between 2003 and 2008. The corr
Externí odkaz:
http://arxiv.org/abs/1410.7435
Autor:
Vucetic, M. M., Arbutina, B., Urosevic, D., Dobardzic, A., Pavlovic, M. Z., Pannuti, T. G., Petrov, N.
Publikováno v:
Serb. Astron. J., vol. 187, pp. 11-18 (2013)
We present observations of the portion of the nearby spiral galaxy IC342 using narrow band [SII] and H$\alpha$ filters. These observations were carried out in November 2011 with the 2m RCC telescope at Rozhen National Astronomical Observatory in Bulg
Externí odkaz:
http://arxiv.org/abs/1312.1510
NGC 7793 - S26 is an extended source (350 pc $\times$ 185 pc) previously studied in the radio, optical and x-ray domains. It has been identified as a micro-quasar which has inflated a super bubble. We used Integral Field Spectra from the Wide Field S
Externí odkaz:
http://arxiv.org/abs/1208.3500