The JCMT BISTRO Survey:The Magnetic Field of the Barnard 1 Star-forming Region

Autor: Coude, S, Bastien, P, Houde, M, Sadavoy, S, Friesen, R, Di Francesco, J, Johnstone, D, Mairs, S, Hasegawa, T, Kwon, W, Lai, S-P, Qiu, K, Ward-Thompson, D, Berry, D, Chen, MC-Y, Fiege, J, Franzmann, E, Hatchell, J, Lacaille, K, Matthews, BC, Moriarty-Schieven, GH, Pon, A, Andre, P, Arzoumanian, D, Aso, Y, Byun, D-Y, Eswaraiah, C, Chen, H-R, Chen, WP, Ching, T-C, Cho, J, Choi, M, Chrysostomou, A, Chung, EJ, Doi, Y, Drabek-Maunder, E, Dowell, CD, Eyres, SPS, Falle, S, Friberg, P, Fuller, G, Furuya, RS, Gledhill, T, Graves, SF, Greaves, JS, Griffin, MJ, Gu, Q, Hayashi, SS, Hoang, T, Holland, W, Inoue, T, Inutsuka, S-I, Iwasaki, K, Jeong, I-G, Kanamori, Y, Kataoka, A, Kang, J-H, Kang, M, Kang, S-J, Kawabata, KS, Kemper, F, Kim, G, Kim, J, Kim, K-T, Kim, KH, Kim, M-R, Kim, S, Kirk, JM, Kobayashi, MIN, Koch, PM, Kwon, J, Lee, J-E, Lee, CW, Lee, S-S, Li, D, Li, H-B, Liu, H-L, Liu, J, Liu, S-Y, Liu, T, van Loo, S, Lyo, A-R, Matsumura, M, Nagata, T, Nakamura, F, Nakanishi, H, Ohashi, N, Onaka, T, Parsons, H, Pattle, K, Peretto, N, Pyo, T-S, Qian, L, Rao, R, Rawlings, MG, Retter, B, Richer, J, Rigby, A, Robitaille, J-F, Saito, H, Savini, G, Scaife, AMM, Seta, M, Shinnaga, H, Soam, A, Tamura, M, Tang, Y-W, Tomisaka, K, Tsukamoto, Y, Wang, H, Wang, J-W, Whitworth, AP, Yen, H-W, Yoo, H, Yuan, J, Zenko, T, Zhang, C-P, Zhang, G, Zhou, J, Zhu, L, The BISTRO Collaboration

Publikováno v: B-Fields In Star-Forming Regions Observations bistro Collaboration, T, Coudé, S, Bastien, P, Houde, M, Sadavoy, S, Friesen, R, Francesco, J D, Johnstone, D, Mairs, S, Hasegawa, T, Kwon, W, Lai, S P, Qiu, K, Ward-Thompson, D, Berry, D, Chen, M C Y, Fiege, J, Franzmann, E, Hatchell, J, Lacaille, K, Matthews, B C, Moriarty-Schieven, G H, Pon, A, André, P, Arzoumanian, D, Aso, Y, Byun, D Y, Eswaraiah, C, Chen, H R, Chen, W P, Ching, T C, Cho, J, Choi, M, Chrysostomou, A, Chung, E J, Doi, Y, Drabek-Maunder, E, Dowell, C D, Eyres, S P S, Falle, S, Friberg, P, Fuller, G, Furuya, R S, Gledhill, T, Graves, S F, Greaves, J S, Griffin, M J, Gu, Q, Hayashi, S S, Hoang, T, Holland, W, Inoue, T, Inutsuka, S I, Iwasaki, K, Jeong, I G, Kanamori, Y, Kataoka, A, Kang, J H, Kang, M, Kang, S J, Kawabata, K S, Kemper, F, Kim, G, Kim, J, Kim, K T, Kim, K H, Kim, M R, Kim, S, Kirk, J M, Kobayashi, M I N, Koch, P M, Kwon, J, Lee, J E, Lee, C W, Lee, S S, Li, D, Li, D, Li, H B, Liu, H L, Liu, J, Liu, S Y, Liu, T, Loo, S V, Lyo, A R, Matsumura, M, Nagata, T, Nakamura, F, Nakanishi, H, Ohashi, N, Onaka, T, Parsons, H, Pattle, K, Peretto, N, Pyo, T S, Qian, L, Rao, R, Rawlings, M G, Retter, B, Richer, J, Rigby, A, Robitaille, J F, Saito, H, Savini, G, Scaife, A M M, Seta, M, Shinnaga, H, Soam, A, Tamura, M, Tang, Y W, Tomisaka, K, Tsukamoto, Y, Wang, H, Wang, J W, Whitworth, A P, Yen, H W, Yoo, H, Yuan, J, Zenko, T, Zhang, C P, Zhang, G, Zhou, J & Zhu, L 2019, ' The JCMT BISTRO Survey : The Magnetic Field of the Barnard 1 Star-forming Region ', Astrophysical Journal, vol. 877, no. 2, 88 . https://doi.org/10.3847/1538-4357/ab1b23
ASTROPHYSICAL JOURNAL

著者人数: The B-fields In STar-forming Regions Observations (BISTRO) Collaboration 121名 (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 權, 靜美)
Number of authors: The B-fields In STar-forming Regions Observat

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7d39c38cb3ab5316952bb3ee19a9d52b
https://doi.org/10.3847/1538-4357/ab1b23

First Results from BISTRO: A SCUBA-2 Polarimeter Survey of the Gould Belt

Autor: Ward-Thompson, D, Pattle, K, Bastien, P, Furuya, RS, Kwon, W, Lai, SP, Qiu, K, Berry, D, Choi, M, Coudé, S, Francesco, JD, Hoang, T, Franzmann, E, Friberg, P, Graves, SF, Greaves, JS, Houde, M, Johnstone, D, Kirk, JM, Koch, PM, Kwon, J, Lee, CW, Li, D, Matthews, BC, Mottram, JC, Parsons, H, Pon, A, Rao, R, Rawlings, M, Shinnaga, H, Sadavoy, S, Loo, SV, Aso, Y, Byun, DY, Eswaraiah, C, Chen, HR, Chen, MCY, Chen, WP, Ching, TC, Cho, J, Chrysostomou, A, Chung, EJ, Doi, Y, Drabek-Maunder, E, Eyres, SPS, Fiege, J, Friesen, RK, Fuller, G, Gledhill, T, Griffin, MJ, Gu, Q, Hasegawa, T, Hatchell, J, Hayashi, SS, Holland, W, Inoue, T, Inutsuka, SI, Iwasaki, K, Jeong, IG, Kang, JH, Kang, M, Kang, SJ, Kawabata, KS, Kemper, F, Kim, G, Kim, J, Kim, KT, Kim, KH, Kim, MR, Kim, S, Lacaille, KM, Lee, JE, Lee, SS, Li, HB, Liu, HL, Liu, J, Liu, SY, Liu, T, Lyo, AR, Mairs, S, Matsumura, M, Moriarty-Schieven, GH, Nakamura, F, Nakanishi, H, Ohashi, N, Onaka, T, Peretto, N, Pyo, TS, Qian, L, Retter, B, Richer, J, Rigby, A, Robitaille, JF, Savini, G, Scaife, AMM, Soam, A, Tamura, M, Tang, YW, Tomisaka, K

We present the first results from the B-fields In STar-forming Region Observations (BISTRO) survey, using the Sub-millimetre Common-User Bolometer Array 2 camera, with its associated polarimeter (POL-2), on the James Clerk Maxwell Telescope in Hawaii

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96e7efa4391030d5fb67069b9c35e85d
https://www.repository.cam.ac.uk/handle/1810/291993

A large light-mass component of cosmic rays at 1017-1017.5 electronvolts from radio observations

Autor: Buitink, S, Corstanje, A, Falcke, H, Hörandel, JR, Huege, T, Nelles, A, Rachen, JP, Rossetto, L, Schellart, P, Scholten, O, Ter Veen, S, Thoudam, S, Trinh, TNG, Anderson, J, Asgekar, A, Avruch, IM, Bell, ME, Bentum, MJ, Bernardi, G, Best, P, Bonafede, A, Breitling, F, Broderick, JW, Brouw, WN, Brüggen, M, Butcher, HR, Carbone, D, Ciardi, B, Conway, JE, De Gasperin, F, De Geus, E, Deller, A, Dettmar, RJ, Van Diepen, G, Duscha, S, Eislöffel, J, Engels, D, Enriquez, JE, Fallows, RA, Fender, R, Ferrari, C, Frieswijk, W, Garrett, MA, Grießmeier, JM, Gunst, AW, Van Haarlem, MP, Hassall, TE, Heald, G, Hessels, JWT, Hoeft, M, Horneffer, A, Iacobelli, M, Intema, H, Juette, E, Karastergiou, A, Kondratiev, VI, Kramer, M, Kuniyoshi, M, Kuper, G, Van Leeuwen, J, Loose, GM, Maat, P, Mann, G, Markoff, S, McFadden, R, McKay-Bukowski, D, McKean, JP, Mevius, M, Mulcahy, DD, Munk, H, Norden, MJ, Orru, E, Paas, H, Pandey-Pommier, M, Pandey, VN, Pietka, M, Pizzo, R, Polatidis, AG, Reich, W, Röttgering, HJA, Scaife, AMM, Schwarz, DJ, Serylak, M, Sluman, J, Smirnov, O, Stappers, BW, Steinmetz, M, Stewart, A, Swinbank, J, Tagger, M, Tang, Y, Tasse, C, Toribio, MC, Vermeulen, R, Vocks, C, Vogt, C, Van Weeren, RJ, Wijers, RAMJ, Wijnholds, SJ, Wise, MW

© 2016 Macmillan Publishers Limited. All rights reserved. Cosmic rays are the highest-energy particles found in nature. Measurements of the mass composition of cosmic rays with energies of 1017-1018 electronvolts are essential to understanding wheth

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od_______363::9d6e0fc1f331862f51f56bccc73544cd
https://hdl.handle.net/10453/113562

Constraining the nature of DG Tau A’s thermal and non-thermal radio emission

Autor: Purser, SJD, Ainsworth, RE, Ray, TP, Green, DA, Taylor, AM, Scaife, AMM

DG Tau A, a class-II young stellar object (YSO) displays both thermal, and non-thermal, radio emission associated with its bipolar jet. To investigate the nature of this emission, we present sensitive (sigma ~ 2 microJy/beam), Karl G.\ Jansky Very La

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::0dbaef3e12245fa3e2b77349b61bbe21

A radio ridge connecting two galaxy clusters in a filament of the cosmic web.

Autor: Govoni F; Istituto Nazionale di Astrofisica-Osservatorio Astronomico di Cagliari Via della Scienza 5, I09047 Selargius, Italy. federica.govoni@inaf.it., Orrù E; ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA, Dwingeloo, Netherlands., Bonafede A; Istituto Nazionale di Astrofisica-Istituto di Radioastronomia, Bologna Via Gobetti 101, I40129 Bologna, Italy.; Dipartimento di Fisica e Astronomia, Università degli Studi di Bologna, Via Gobetti 93/2, I40129 Bologna, Italy.; Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany., Iacobelli M; ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA, Dwingeloo, Netherlands., Paladino R; Istituto Nazionale di Astrofisica-Istituto di Radioastronomia, Bologna Via Gobetti 101, I40129 Bologna, Italy., Vazza F; Istituto Nazionale di Astrofisica-Istituto di Radioastronomia, Bologna Via Gobetti 101, I40129 Bologna, Italy.; Dipartimento di Fisica e Astronomia, Università degli Studi di Bologna, Via Gobetti 93/2, I40129 Bologna, Italy.; Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany., Murgia M; Istituto Nazionale di Astrofisica-Osservatorio Astronomico di Cagliari Via della Scienza 5, I09047 Selargius, Italy., Vacca V; Istituto Nazionale di Astrofisica-Osservatorio Astronomico di Cagliari Via della Scienza 5, I09047 Selargius, Italy., Giovannini G; Istituto Nazionale di Astrofisica-Istituto di Radioastronomia, Bologna Via Gobetti 101, I40129 Bologna, Italy.; Dipartimento di Fisica e Astronomia, Università degli Studi di Bologna, Via Gobetti 93/2, I40129 Bologna, Italy., Feretti L; Istituto Nazionale di Astrofisica-Istituto di Radioastronomia, Bologna Via Gobetti 101, I40129 Bologna, Italy., Loi F; Istituto Nazionale di Astrofisica-Osservatorio Astronomico di Cagliari Via della Scienza 5, I09047 Selargius, Italy.; Dipartimento di Fisica e Astronomia, Università degli Studi di Bologna, Via Gobetti 93/2, I40129 Bologna, Italy., Bernardi G; Istituto Nazionale di Astrofisica-Istituto di Radioastronomia, Bologna Via Gobetti 101, I40129 Bologna, Italy.; Department of Physics and Electronics, Rhodes University, Grahamstown, South Africa.; Square Kilometre Array South Africa, 3rd Floor, The Park, Park Road, Pinelands 7405, South Africa., Ferrari C; Université Côte d'Azur, Observatoire de la Côte d'Azur, Centre National de la Recherche Scientifique, Laboratoire Lagrange, Blvd. de l'Observatoire, CS 34229, 06304 Nice Cedex 4, France., Pizzo RF; ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA, Dwingeloo, Netherlands., Gheller C; Swiss Plasma Center, Ecole Polytechnique Fédérale de Lausanne, 1015 Ecublens, Lausanne, Switzerland., Manti S; Scuola Normale Superiore, Piazza dei Cavalieri 7, I-56126 Pisa, Italy., Brüggen M; Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany., Brunetti G; Istituto Nazionale di Astrofisica-Istituto di Radioastronomia, Bologna Via Gobetti 101, I40129 Bologna, Italy., Cassano R; Istituto Nazionale di Astrofisica-Istituto di Radioastronomia, Bologna Via Gobetti 101, I40129 Bologna, Italy., de Gasperin F; Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany.; Leiden University, Rapenburg 70, 2311 EZ Leiden, Netherlands., Enßlin TA; Max Planck Institut für Astrophysik, Karl-Schwarzschild-Str.1, D-85740 Garching, Germany.; Ludwig-Maximilians-Universität München, Geschwister-Scholl-Platz 1, D-80539, München, Germany., Hoeft M; Thüringer Landessternwarte, Sternwarte 5, 07778 Tautenburg, Germany., Horellou C; Chalmers University of Technology, Dept. of Space, Earth and Environment, Onsala Space Observatory, SE-439 92 Onsala, Sweden., Junklewitz H; Argelander Institut für Astronomie, Auf dem Hügel, 71 D-53121 Bonn, Germany., Röttgering HJA; Leiden University, Rapenburg 70, 2311 EZ Leiden, Netherlands., Scaife AMM; Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester M13 9PL, UK., Shimwell TW; ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA, Dwingeloo, Netherlands.; Leiden University, Rapenburg 70, 2311 EZ Leiden, Netherlands., van Weeren RJ; Leiden University, Rapenburg 70, 2311 EZ Leiden, Netherlands., Wise M; ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA, Dwingeloo, Netherlands.; SRON Netherlands Institute for Space Research Sorbonnelaan 2, 3584 CA Utrecht, Netherlands.

Publikováno v: Science (New York, N.Y.) [Science] 2019 Jun 07; Vol. 364 (6444), pp. 981-984.