Zobrazeno 1 - 10
of 4 917
pro vyhledávání: '"Maxted, N"'
Autor:
Yamane, Y., Sano, H., Filipovic, M. D., Tokuda, K., Fujii, K., Babazaki, Y., Mitsuishi, I., Inoue, T., Aharonian, F., Inaba, T., Inutsuka, S., Maxted, N., Mizuno, N., Onishi, T., Rowell, G., Tsuge, K., Voisin, F., Yoshiike, S., Fukuda, T., Kawamura, A., Bamba, A., Tachihara, K., Fukui, Y.
30 Doradus C is a superbubble which emits the brightest nonthermal X- and TeV gamma-rays in the Local Group. In order to explore detailed connection between the high energy radiation and the interstellar medium, we have carried out new CO and HI obse
Externí odkaz:
http://arxiv.org/abs/2106.09916
Autor:
Feijen, K., Rowell, G., Einecke, S., Braiding, C., Burton, M. G., Maxted, N., Voisin, F., Wong, G. F.
The Galactic TeV $\gamma$-ray source HESS$\,$J1804$-$216 is currently an unidentified source. In an attempt to unveil its origin, we present here the most detailed study of interstellar gas using data from the Mopra Southern Galactic Plane CO Survey,
Externí odkaz:
http://arxiv.org/abs/2011.09021
Autor:
Sano, H., Inoue, T., Tokuda, K., Tanaka, T., Yamazaki, R., Inutsuka, S., Aharonian, F., Rowell, G., Filipovic, M. D., Yamane, Y., Yoshiike, S., Maxted, N., Uchida, H., Hayakawa, T., Tachihara, K., Uchiyama, Y., Fukui, Y.
RX J1713.7-3946 is a unique core-collapse SNR that emits bright TeV gamma-rays and synchrotron X-rays caused by cosmic rays, in addition to interactions with interstellar gas clouds. We report here on results of ALMA $^{12}$CO($J$ = 1-0) observations
Externí odkaz:
http://arxiv.org/abs/2011.05018
Energy released when the core of a high-mass star collapses into a black hole often powers an explosion that creates a supernova remnant. Black holes have limited windows of observability, and consequently are rarely identified in association with su
Externí odkaz:
http://arxiv.org/abs/2010.15341
Autor:
Sano, H., Plucinsky, P. P., Bamba, A., Sharda, P., Filipovic, M. D., Law, C. J., Alsaberi, R. Z. E., Yamane, Y., Tokuda, K., Acero, F., Sasaki, M., Vink, J., Inoue, T., Inutsuka, S., Shimoda, J., Tsuge, K., Fujii, K., Voisin, F., Maxted, N., Rowell, G., Onishi, T., Kawamura, A., Mizuno, N., Yamamoto, H., Tachihara, K., Fukui, Y.
Publikováno v:
The Astrophysical Journal, 902, 53 (2020)
N132D is the brightest gamma-ray supernova remnant (SNR) in the Large Magellanic Cloud (LMC). We carried out $^{12}$CO($J$ = 1-0, 3-2) observations toward the SNR using the Atacama Large Millimeter/submillimeter Array (ALMA) and Atacama Submillimeter
Externí odkaz:
http://arxiv.org/abs/2007.07900
Autor:
Alsaberi, R. Z. E., Barnes, L. A., Filipovic, M. D., Maxted, N. I., Sano, H., Rowell, G., Bozzetto, L. M., Gurovich, S., Urovsevic, D., Onic, D., For, B. Q., Manojlovic, P., Wong, G., Galvin, T., Kavanagh, P., Ralph, N., Crawford, E. J., Sasaki, M., Haberl, F., Maggi, P., Tothil, N. F. H., Fukui, Y.
Here we present a radio continuum study based on new and archival data from the Australia Telescope Compact Array towards N 103B, a young (<=1000 yrs) spectroscopically confirmed type Ia SNR in the Large Magellanic Cloud (LMC) and proposed to have or
Externí odkaz:
http://arxiv.org/abs/1911.04051
Autor:
Joseph, T. D., Filipović, M. D., Crawford, E. J., Bojičić, I., Alexander, E. L., Wong, G. F., Andernach, H., Leverenz, H., Norris, R. P., Alsaberi, R. Z. E., Anderson, C., Barnes, L. A., Bozzetto, L. M., Bufano, F., Bunton, J. D., Cavallaro, F., Collier, J. D., Dénes, H., Fukui, Y., Galvin, T., Haberl, F., Ingallinera, A., Kapinska, A. D., Koribalski, B. S., Kothes, R., Li, D., Maggi, P., Maitra, C., Manojlović, P., Marvil, J., Maxted, N. I., Brien, A. N. O, Oliveira, J. M., Pennock, C. M., Riggi, S., Rowell, G., Rudnick, L., Sano, H., Sasaki, M., Seymour, N., Soria, R., Stupar, M., Tothill, N. F. H., Trigilio, C., Tsuge, K., Umana, G., Urošević, D., van Loon, J. Th., Vardoulaki, E., Velović, V., Yew, M., Leahy, D., Chu, Y. -H., Micha\{l}owski, M. J., Kavanagh, P. J., Grieve, K. R.
We present two new radio continuum images from the Australian Square Kilometre Array Pathfinder (ASKAP) survey in the direction of the Small Magellanic Cloud (SMC). These images are part of the Evolutionary Map of the Universe (EMU) Early Science Pro
Externí odkaz:
http://arxiv.org/abs/1909.10425
Autor:
Voisin, F. J., Rowell, G. P., Burton, M. G., Fukui, Y., Sano, H., Aharonian, F., Maxted, N., Braiding, C., Blackwell, R., Lau, J.
Publikováno v:
Publications of the Astronomical Society of Australia, 36, E014 (2019)
We investigate the interstellar medium (ISM) towards seven TeV gamma-ray sources thought to be pulsar wind nebulae (PWNe) using Mopra molecular line observations at 7mm [CS(1-0), SiO(1-0,v=0)], Nanten CO(1-0) data and the SGPS/GASS HI survey. We have
Externí odkaz:
http://arxiv.org/abs/1905.04517
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
Autor:
Sano, H., Matsumura, H., Yamane, Y., Maggi, P., Fujii, K., Tsuge, K., Tokuda, K., Alsaberi, R. Z. E., Filipovic, M. D., Maxted, N., Rowell, G., Uchida, H., Tanaka, T., Muraoka, K., Takekoshi, T., Onishi, T., Kawamura, A., Minamidani, T., Mizuno, N., Yamamoto, H., Tachihara, K., Inoue, T., Inutsuka, S., Voisin, F., Tothill, N. F. H., Sasaki, M., McClure-Griffiths, N. M., Fukui, Y.
RX J0046.5$-$7308 is a shell-type supernova remnant (SNR) in the Small Magellanic Cloud (SMC). We carried out new $^{12}$CO($J$ = 1-0, 3-2) observations toward the SNR using Mopra and the Atacama Submillimeter Telescope Experiment. We found eight mol
Externí odkaz:
http://arxiv.org/abs/1904.04836