Search Results - "Rowell, G"

ALMA CO Observations of the Mixed-morphology Supernova Remnant W49B: Efficient Production of Recombining Plasma and Hadronic Gamma Rays via Shock–Cloud Interactions by Sano, H., Yoshiike, S., Yamane, Y., Hayashi, K., Enokiya, R., Tokuda, K., Tachihara, K., Rowell, G., Filipović, M. D., Fukui, Y.

“…Abstract We carried out new CO( J = 2–1) observations toward the mixed-morphology supernova remnant (SNR) W49B with the Atacama Large Millimeter/submillimeter…”
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Using interstellar clouds to search for Galactic PeVatrons: gamma-ray signatures from supernova remnants by Mitchell, A M W, Rowell, G P, Celli, S, Einecke, S

“…ABSTRACT Interstellar clouds can act as target material for hadronic cosmic rays; gamma rays subsequently produced through inelastic proton–proton collisions…”
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ISM gas studies towards the TeV PWN HESS J1825−137 and northern region by Voisin, F., Rowell, G., Burton, M. G., Walsh, A., Fukui, Y., Aharonian, F.

“…HESS J1825−137 is a pulsar wind nebula (PWN) whose TeV emission extends across ∼1 $\deg$ . Its large asymmetric shape indicates that its progenitor supernova…”
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Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Puppis A by Aruga, M., Sano, H., Fukui, Y., Reynoso, E. M., Rowell, G., Tachihara, K.

“…Abstract We have carried out a study of the interstellar medium (ISM) toward the shell-like supernova remnant (SNR) Puppis A using NANTEN CO and ATCA H i data…”
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A 3D diffusive and advective model of electron transport applied to the pulsar wind nebula HESS J1825 − 137 by Collins, T, Rowell, G, Einecke, S, Voisin, F, Fukui, Y, Sano, H

“…ABSTRACT HESS J1825 − 137 is one of the most powerful and luminous TeV gamma-ray pulsar wind nebulae, making it an excellent laboratory to study particle…”
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The steady-state multi-TeV diffuse γ-ray emission predicted with galprop and prospects for the Cherenkov Telescope Array by Marinos, P D, Rowell, G P, Porter, T A, Jóhannesson, G

“…ABSTRACT Cosmic rays (CRs) interact with the diffuse gas, radiation, and magnetic fields in the interstellar medium (ISM) to produce electromagnetic emissions…”
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An Expanding Shell of Neutral Hydrogen Associated with SN 1006: Hints for the Single-degenerate Origin and Faint Hadronic Gamma-Rays by Sano, H., Yamaguchi, H., Aruga, M., Fukui, Y., Tachihara, K., Filipović, M. D., Rowell, G.

“…Abstract We report new H i observations of the Type Ia supernova remnant (SNR) SN 1006 using the Australia Telescope Compact Array with an angular resolution…”
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ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons by Sano, H., Plucinsky, P. P., Bamba, A., Sharda, P., Filipovi, 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.

“…N132D is the brightest gamma-ray supernova remnant (SNR) in the Large Magellanic Cloud (LMC). We carried out 12CO(J = 1-0, 3-2) observations toward the SNR…”
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The ASKAP EMU Early Science Project: radio continuum survey of the Small Magellanic Cloud by 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, O’Brien, A N, 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, Michałowski, M J, Kavanagh, P J, Grieve, K R

“…ABSTRACT We present two new radio continuum images from the Australian Square Kilometre Array Pathfinder (ASKAP) survey in the direction of the Small…”
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Modelling the gamma-ray morphology of HESSJ1804−216 from two supernova remnants in a hadronic scenario by Feijen, K, Einecke, S, Rowell, G, Braiding, C, Burton, M G, Wong, G F

“…ABSTRACT HESS J1804−216 is one of the brightest yet most mysterious TeV γ-ray sources discovered to date. Previous arc-minute scale studies of the interstellar…”
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Explaining the extended GeV gamma-ray emission adjacent to HESS J1825-137 by Collins, T, Rowell, G, Mitchell, A M W, Voisin, F, Fukui, Y, Sano, H, Alsulami, R, Einecke, S

“…ABSTRACT HESS J1825-137 is one of the most powerful and luminous TeV gamma-ray pulsar wind nebulae (PWN). To the south of HESS J1825-137, Fermi-LAT observation…”
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Probing the local environment of the supernova remnant HESS J1731−347 with CO and CS observations by Maxted, N., Burton, M., Braiding, C., Rowell, G., Sano, H., Voisin, F., Capasso, M., Pühlhofer, G., Fukui, Y.

“…Abstract The shell-type supernova remnant HESS J1731 − 347 emits TeV gamma-rays, and is a key object for the study of the cosmic ray acceleration potential of…”
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ALMA Observations of Supernova Remnant N49 in the Large Magellanic Cloud. II. Non-LTE Analysis of Shock-heated Molecular Clouds by Sano, H., Yamane, Y., van Loon, J. Th, Furuya, K., Fukui, Y., Alsaberi, R. Z. E., Bamba, A., Enokiya, R., Filipović, M. D., Indebetouw, R., Inoue, T., Kawamura, A., Lakićević, M., Law, C. J., Mizuno, N., Murase, T., Onishi, T., Park, S., Plucinsky, P. P., Rho, J., Richards, A. M. S., Rowell, G., Sasaki, M., Seok, J., Sharda, P., Staveley-Smith, L., Suzuki, H., Temim, T., Tokuda, K., Tsuge, K., Tachihara, K.

“…Abstract We present the first compelling evidence of shock-heated molecular clouds associated with the supernova remnant (SNR) N49 in the Large Magellanic…”
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A DETAILED STUDY OF THE MOLECULAR AND ATOMIC GAS TOWARD THE γ-RAY SUPERNOVA REMNANT RX J1713.7―3946: SPATIAL TeV γ-RAY AND INTERSTELLAR MEDIUM GAS CORRESPONDENCE by FUKUI, Y, SANO, H, KAWAMURA, A, YAMAMOTO, H, OKUDA, T, MIZUNO, N, ONISHI, T, MIZUNO, A, OGAWA, H, SATO, J, TORII, K, HORACHI, H, HAYAKAWA, T, MCCLURE-GRIFFITHS, N. M, ROWELL, G, INOUE, T, INUTSUKA, S

“…RX J1713.7-3946 is the most remarkable TeV gamma -ray supernova remnant (SNR) that emits gamma -rays in the highest energy range. We have made a new combined…”
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Possible Evidence for Cosmic-Ray Acceleration in the Type Ia SNR RCW 86: Spatial Correlation between TeV Gamma-Rays and Interstellar Atomic Protons by Sano, H., Rowell, G., Reynoso, E. M., Jung-Richardt, I., Yamane, Y., Nagaya, T., Yoshiike, S., Hayashi, K., Torii, K., Maxted, N., Mitsuishi, I., Inoue, T., Inutsuka, S., Yamamoto, H., Tachihara, K., Fukui, Y.

“…We present a detailed morphological study of TeV gamma-rays, synchrotron radiation, and interstellar gas in the young Type Ia supernova remnant (SNR) RCW 86…”
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A Detailed Study of the Interstellar Protons toward the TeV γ-Ray SNR RX J0852.0-4622 (G266.2-1.2, Vela Jr.): The Third Case of the γ-Ray and ISM Spatial Correspondence by Fukui, Y., Sano, H., Sato, J., Okamoto, R., Fukuda, T., Yoshiike, S., Hayashi, K., Torii, K., Hayakawa, T., Rowell, G., Filipovi, M. D., Maxted, N., McClure-Griffiths, N. M., Kawamura, A., Yamamoto, H., Okuda, T., Mizuno, N., Tachihara, K., Onishi, T., Mizuno, A., Ogawa, H.

“…We present a new analysis of the interstellar protons toward the TeV γ-ray SNR RX J0852.0−4622 (G266.2−1.2, Vela Jr.). We used the NANTEN2 12CO(J = 1-0) and…”
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A Morphological Study of the Supernova Remnant Rx J0852.0-4622 (Vela Jr.) by Maxted, Nigel I., Filipovi, 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., Manojlovi, P., O'Brien, A.

“…We conduct a multiwavelength morphological study of the Galactic supernova remnant (SNR) RX J0852.0-4622 (also known as Vela Jr., Vela Z, and G266.2−1.2). RX…”
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New ASKAP radio supernova remnants and candidates in the Large Magellanic Cloud by Bozzetto, Luke M, Filipović, Miroslav D, Sano, H, Alsaberi, R Z E, Barnes, L A, Bojičić, I S, Brose, R, Chomiuk, L, Crawford, E J, Dai, S, Ghavam, M, Haberl, F, Hill, T, Hopkins, A M, Ingallinera, A, Jarrett, T, Kavanagh, P J, Koribalski, B S, Kothes, R, Leahy, D, Lenc, E, Leonidaki, I, Maggi, P, Maitra, C, Matthew, C, Payne, J L, Pennock, C M, Points, S, Reid, W, Riggi, S, Rowell, G, Sasaki, M, Safi-Harb, S, van Loon, J Th, Tothill, N F H, Urošević, D, Zangrandi, F

“…ABSTRACT We present a new Australian Square Kilometre Array Pathfinder (ASKAP) sample of 14 radio supernova remnants (SNR) candidates in the Large Magellanic…”
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Searching for an interstellar medium association for HESS J1534 − 571 by Maxted, Nigel I, Braiding, C, Wong, G F, Rowell, G P, Burton, M G, Filipović, M D, Voisin, F, Urošević, D, Vukotić, B, Pavlović, M Z, Sano, H, Fukui, Y

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Discovery of Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Kesteven 79 by Kuriki, M., Sano, H., Kuno, N., Seta, M., Yamane, Y., Inaba, T., Nagaya, T., Yoshiike, S., Okawa, K., Tsutsumi, D., Hattori, Y., Kohno, M., Fujita, S., Nishimura, A., Ohama, A., Matsuo, M., Tsuda, Y., Torii, K., Minamidani, T., Umemoto, T., Rowell, G., Bamba, A., Tachihara, K., Fukui, Y.

“…We carried out 12CO(J = 1-0) observations of the Galactic gamma-ray supernova remnant (SNR) Kesteven 79 using the Nobeyama Radio Observatory 45 m radio…”
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