Origin of the galactic Centre lobes
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Mid-IR observations at 8, 12, and 22 μm support the idea of shocks.
“This idea of the shock is indeed supported by mid-IR observations at 8 µ m, 12 µ m, and 22 µ m (Uchida et al. 1985; Shibata & Uchida 1987; Bland-Hawthorn & Cohen 2003; Ponti et al. 2021).”
From The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way (2024) · cites this paper as Uchida et al. 1985
Cites
Hydromagnetic flows from accretion discs and the production of radio jets
Blandford, R. D., & Payne, D. G. (1982) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/199.4.883 · Cited by 4,109 · see citing works
Theory of extragalactic radio sources
Begelman, M. C., Blandford, R. D., & Rees, M. J. (1984) · Reviews of Modern Physics · doi:10.1103/revmodphys.56.255 · Cited by 1,707 · see citing works
A 'Twin-Exhaust' Model for Double Radio Sources
Blandford, R. D., & Rees, M. J. (1974) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/169.3.395 · Cited by 773 · see citing works
Large, highly organized radio structures near the galactic centre
Yusef-Zadeh, F., Morris, M., & Chance, D. (1984) · Nature · doi:10.1038/310557a0 · Cited by 379 · see citing works
Centrifugally driven winds from contracting molecular disks
Pudritz, R. E., & Norman, C. A. (1983) · The Astrophysical Journal · doi:10.1086/161481 · Cited by 350 · see citing works
A radio lobe over the galactic centre
Sofue, Y., & Handa, T. (1984) · Nature · doi:10.1038/310568a0 · Cited by 175 · see citing works
Self-citationOn the nature of bipolar sources in dense molecular clouds
Königl, A. (1982) · The Astrophysical Journal · doi:10.1086/160324 · Cited by 152 · see citing works
Magnetic field structure in the vicinity of five dark cloud complexes
Vrba, F. J., Strom, S. E., & Strom, K. M. (1976) · The Astronomical Journal · doi:10.1086/111976 · Cited by 141 · see citing works
Magnetic bubbles and high-velocity outflows in molecular clouds
Draine, B. T. (1983) · The Astrophysical Journal · doi:10.1086/161145 · Cited by 54 · see citing works
An Electrodynamic Model of Radio Galaxies and Quasars
Piddington, J. H. (1970) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/148.2.131 · Cited by 35 · see citing works
Magnetic braking of self-gravitating, oblate interstellar clouds
Mouschovias, T. C. (1979) · The Astrophysical Journal · doi:10.1086/156832 · Cited by 32 · see citing works
HII Regions and Star Formation in the Galactic Center
Mezger, P. G., & Pauls, T. A. (1979) · Springer eBooks · doi:10.1007/978-94-009-9503-1_66 · Cited by 31 · see citing works
The magnetic field of a rotating cloud and magneto-rotational explosions
Ozernoy, L. M., & Somov, B. V. (1971) · Astrophysics and Space Science · doi:10.1007/bf00661358 · Cited by 29 · see citing works
Molecules in the Inner Few KPC of the Galaxy
Liszt, H. S., & Burton, W. B. (1979) · Springer eBooks · doi:10.1007/978-94-009-9503-1_64 · Cited by 1 · see citing works
Flagged first, then by citations
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THE GALACTIC CENTER ENVIRONMENT
Morris, M., & Serabyn, E. (1996) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.34.1.645 · Cited by 930 · see citing works
“Another alternative is that the NTFs lie upon the surface of a cylindrical wall of compressed magnetic field surrounding the Galactic center (Uchida et al 1985, Heyvaerts et al 1988) and that they are again illuminated by some local mechanism for the generation of relativistic particles.”
BackgroundMethodA Wide-Field 90 Centimeter VLA Image of the Galactic Center Region
LaRosa, T. N., Kassim, N. E., Lazio, T. J. W., & Hyman, S. D. (2000) · The Astronomical Journal · doi:10.1086/301168 · Cited by 195 · see citing works
The Galactic Center Molecular Cloud Survey
Kauffmann, J., Pillai, T., Zhang, Q., Menten, K. M., Goldsmith, P. F., Lu, X., & Guzmán, A. E. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201628088 · Cited by 134 · see citing works
“The gas is pervaded by a strong magnetic field of a few 103 µG (Yusef-Zadeh et al. 1984; Uchida et al. 1985; Chuss et al. 2003; Novak et al. 2003) that also penetrates the CMZ clouds (Pillai et al. 2015).”
BackgroundThe <i>XMM–Newton</i> view of the central degrees of the Milky Way
Ponti, G., Morris, M. R., Terrier, R., Haberl, F., Sturm, R., Clavel, M., Soldi, S., Goldwurm, A., Predehl, P., Nandra, K., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1331 · Cited by 125 · see citing works
“This opens the exciting possibility that the observed high-latitude enhanced X-ray emission from the GC ”atmosphere” is indeed the warm plasma filling the GCL. Based on the spectral fit, we deduce a density of ne = 0.06 cm−3 inside the GCL. Assuming uniform physical conditions inside the GCL (a cylinder of 45 pc radiu…”
BackgroundInfluentialWild at Heart:-The Particle Astrophysics of the Galactic Centre
Crocker, R., Jones, D., Aharonian, F., Law, C., Melia, F., Oka, T., & Ott, J. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.18170.x · Cited by 107 · see citing works
“…in 10 GHz radio continuum emission (Sofue & Handa 1984) and has been interpreted as evidence for a previous episode of either starburst (Chevalier 1992; Bland-Hawthorn & Cohen 2003) or nuclear activity (Kundt 1987; Melia & Falcke 2001) or as due to magnetodynamic effects (Uchida et al. 1985).”
BackgroundSofue, Y. (2000) · The Astrophysical Journal · doi:10.1086/309297 · Cited by 102 · see citing works
Self-citationNovak, G., Chuss, D. T., Renbarger, T., Griffin, G. S., Newcomb, M., Peterson, J. B., Loewenstein, R. F., Pernic, D., & Dotson, J. (2003) · The Astrophysical Journal · doi:10.1086/368156 · Cited by 103 · see citing works
Magnetic Fields in Cool Clouds within the Central 50 Parsecs of the Galaxy
Chuss, D. T., Davidson, J. A., Dotson, J., Dowell, C. D., Hildebrand, R. H., Novak, G., & Vaillancourt, J. E. (2003) · The Astrophysical Journal · doi:10.1086/379538 · Cited by 95 · see citing works
“One possible interpretation of this result relies again on the model of Uchida et al. (1985).”
BackgroundResultOka, T., Geballe, T. R., Goto, M., Usuda, T., Benjamin, J. M., & Indriolo, N. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab3647 · Cited by 85 · see citing works
“More recently a milligauss magnetic field was reported by Chuss et al. (2003) from submillimeter polarimetric observations based on the model calculations of Uchida et al. (1985).”
MethodNew Nonthermal Filaments at the Galactic Center: Are They Tracing a Globally Ordered Magnetic Field?
LaRosa, T. N., Nord, M. E., Joseph, T., Lazio, W., & Kassim, N. E. (2004) · The Astrophysical Journal · doi:10.1086/383233 · Cited by 70 · see citing works
“Ejection or expansion of magnetic fields from an accretion disk (Heyvaerts, Norman, & Pudritz 1998; Uchida et al. 1985) or a shocked Galactic wind (Bland-Hawthorn & Cohen 2003; Chevalier 1992) are possibilities for the origin of these structures.”
BackgroundMAGNETICALLY CONFINED INTERSTELLAR HOT PLASMA IN THE NUCLEAR BULGE OF OUR GALAXY
Nishiyama, S., Yasui, K., Nagata, T., Yoshikawa, T., Uchiyama, H., Schödel, R., Hatano, H., Sato, S., Sugitani, K., Suenaga, T., et al. (2013) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/769/2/l28 · Cited by 34 · see citing works
The Galactic Center Molecular Cloud Survey
Kauffmann, J., Pillai, T., Zhang, Q., Menten, K. M., Goldsmith, P. F., Lu, X., Guzmán, A. E., & Schmiedeke, A. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201628089 · Cited by 51 · see citing works
“The gas is pervaded by a strong magnetic field of a few 103 µG (Yusef-Zadeh et al. 1984; Uchida et al. 1985; Chuss et al. 2003; Novak et al. 2003).”
BackgroundMagnetic field near the central region of the Galaxy: rotation measure of extragalactic sources
Roy, S., Rao, A. P., & Subrahmanyan, R. (2007) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20066470 · Cited by 44 · see citing works
“(i) Magnetohydrodynamic model: Uchida et al. (1985) proposed this model to explain the Galactic Centre Lobes (GCL), which are a pair of limbbrightened radio structures of several hundred parsecs extending from Galactic plane towards positive Galactic latitudes (Sofue & Handa 1984) and seen within…”
MethodCosmic magnetism in centimeter- and meter-wavelength radio astronomy
Akahori, T., Nakanishi, H., Sofue, Y., Fujita, Y., Ichiki, K., Ideguchi, S., Kameya, O., Kudoh, T., Kudoh, Y., Machida, M., et al. (2017) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psx123 · Cited by 44 · see citing works
“An MHD model on the magnetic field structure near the Galactic Center was proposed by Uchida et al. (1985) and extended by Shibata & Uchida (1987).”
MethodSelf-citationKauffmann, J., Pillai, T., Zhang, Q., Menten, K. M., Goldsmith, P. F., Lu, X., & Guzmán, A. E. (2017) · Max Planck Digital Library · Cited by 44 · see citing works
A MULTIWAVELENGTH VIEW OF A MASS OUTFLOW FROM THE GALACTIC CENTER
Law, C. J. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/708/1/474 · Cited by 45 · see citing works
“The shape and location of the shell motivated several models for its formation, including starburst (Chevalier 1992), active galactic nucleus (AGN; Melia & Falcke 2001), and magnetodynamic effects (Uchida et al. 1985).”
BackgroundMethodThe geometry of the magnetic field in the central molecular zone measured by PILOT
Mangilli, A., Aumont, J., Bernard, J.-P., Buzzelli, A., de Gasperis, G., Durrive, J.-B., Ferrière, K., Foënard, G., Hughes, A., Lacourt, A., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201935072 · Cited by 42 · see citing works
“These authors argued that the observed RM pattern could be explained by the model of Uchida et al. (1985), in which an initially vertical magnetic field is sheared out in the azimuthal direction by the differential rotation of the dense clouds present near the Galactic plane.”
BackgroundThe Galactic Center Magnetosphere
Morris, M. (2006) · Journal of Physics Conference Series · doi:10.1088/1742-6596/54/1/001 · Cited by 41 · see citing works
Nishiyama, S., Tamura, M., Hatano, H., Kanai, S., Kurita, M., Sato, S., Matsunaga, N., Nagata, T., Nagayama, T., Kandori, R., et al. (2008) · The Astrophysical Journal · doi:10.1088/0004-637x/690/2/1648 · Cited by 35 · see citing works
“A model that can connect the poloidal and toroidal magnetic fields was proposed by Uchida et al. (1985), and was extended to a more realistic case by Shibata & Uchida (1986).”
The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way
Sarkar, K. C. (2024) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-024-00152-1 · Cited by 34 · see citing works
“This idea of the shock is indeed supported by mid-IR observations at 8 µ m, 12 µ m, and 22 µ m (Uchida et al. 1985; Shibata & Uchida 1987; Bland-Hawthorn & Cohen 2003; Ponti et al. 2021).”
The geometry of the magnetic field in the central molecular zone measured by PILOT
Mangilli, A., Aumont, J., Bernard, J.-P., Buzzelli, A., de Gasperis, G., Durrive, J.-B., Ferrière, K., Foënard, G., Hughes, A., Lacourt, A., et al. (2019) · UCL Discovery (University College London) · Cited by 33 · see citing works
Hsieh, P.-Y., Koch, P. M., Kim, W.-T., Ho, P. T. P., Tang, Y.-W., & Wang, H.-H. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aacb27 · Cited by 33 · see citing works
“Uchida et al. (1985) constructed a model to connect poloidal and toroidal field components based on the assumption of magnetic flux-freezing.”
Radio polarimetry of Galactic Centre pulsars
Schnitzeler, D. H. F. M., Eatough, R. P., Ferrière, K., Krämer, M., Lee, K., Noutsos, A., & Shannon, R. M. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw841 · Cited by 30 · see citing works
“Differential rotation in the GC, leading to a windingup of field lines, was predicted to produce a checkerboard pattern in the sign of RM (Uchida et al. 1985); the RMs of NTFs agreed with one of the two possible solutions for this pattern (e.g., Novak et al. 2003).”
BackgroundMethodThree-Dimensional Global MHD Simulations of Accretion Disks and Jet Formation
Matsumoto, R. (1999) · Astrophysics and space science library · doi:10.1007/978-94-011-4780-4_62 · Cited by 30 · see citing works
Morris, M. (1994) · Springer eBooks · doi:10.1007/978-94-011-0752-5_25 · Cited by 24 · see citing works
Kauffmann, J., Pillai, T., Zhang, Q., Menten, K. M., Goldsmith, P. F., Lu, X., Guzmán, A. E., & Schmiedeke, A. (2017) · Kölner Universitäts PublikationsServer (Universität zu Köln) · Cited by 23 · see citing works
A CONSTRAINT ON THE ORGANIZATION OF THE GALACTIC CENTER MAGNETIC FIELD USING FARADAY ROTATION
Law, C. J., Brentjens, M. A., & Novak, G. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/731/1/36 · Cited by 22 · see citing works
“The checkerboard pattern inspired the “flux-dragging” model for the GC magnetic field (Uchida et al. 1985; Novak et al. 2003).”
MethodResultManifestations of the Galactic Center Magnetic Field
Morris, M. (2014) · Springer eBooks · doi:10.1007/978-3-319-10614-4_32 · Cited by 18 · see citing works
“Soon after the NTFs were discovered (Yusef-Zadeh et al. 1984), Uchida et al. (1985) formulated a model in which gas in the differentially rotating Galactic disk interacts with a globally poloidal field by dragging it into a twisted, toroidal configuration.”
BackgroundThe Magnetic Field in the Inner 70 Parsecs of the Milky Way
Morris, M. (1990) · Springer eBooks · doi:10.1007/978-94-009-0569-6_115 · Cited by 17 · see citing works
The Primordial Origin Model of Magnetic Fields in Spiral Galaxies
Sofue, Y., Machida, M., & Kudoh, T. (2010) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/62.5.1191 · Cited by 15 · see citing works
“This causes a vertical outflow of gas as well as a loss of the angular momentum of the disk by magnetic braking, accelerating the contraction of the galactic disk (Uchida et al. 1985).”
BackgroundSelf-citationHigh-Velocity Molecular Gas in the Galactic Center Radio Lobe
Sofue, Y. (1996) · The Astrophysical Journal · doi:10.1086/309946 · Cited by 11 · see citing works
“The gas -vs-magnetic field location would depend on the initial configuration of the poloidal field and accretion disk, and a detailed modeling is desired (Uchida et al 1985).”
BackgroundMethodSelf-citationParé, D. M., Chuss, D. T., Karpovich, K., Butterfield, N., Iuliano, J. I., Pan, X., Wollack, E. J., Zhang, Q., Morris, M., Nilsson, M., et al. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad9586 · Cited by 9 · see citing works
“We posit that an initial field is sheared into a field oriented parallel to the orbital mo-18 tions of the cloud (e.g., Uchida et al. 1985; Chuss et al. 2003).”
High-Velocity Molecular Gas in the Galactic Center Radio LobePreprint
Sofue, Y. (1995) · Cited by 9 · see citing works
Self-citationMagnetic-Reconnection and Current-Sheet Model for the Radio Arc and Threads in the Galactic Center
Sofue, Y., Kigure, H., & Shibata, K. (2005) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/57.5.l39 · Cited by 7 · see citing works
Self-citationLarge-Scale Radio Structures in the Galactic Center
Sofue, Y. (1994) · Springer eBooks · doi:10.1007/978-94-011-0752-5_5 · Cited by 7 · see citing works
“This will result in a cylindrical outflow of gas and cosmic rays, which will account for the formation of the galactic center lobe (Uchida et al 1985; Uchida and Shibata 1986; Shibata and Uchida 1987).”
BackgroundMethodSelf-citationNumerical Simulation of Solar and Astrophysical MHD Flows
Shibata, K. (1996) · Springer eBooks · doi:10.1007/978-94-009-0265-7_11 · Cited by 6 · see citing works
Self-citationLarge-Scale Ejection Structures in the Galactic Center
Sofue, Y. (1989) · Springer eBooks · doi:10.1007/978-94-009-2362-1_29 · Cited by 6 · see citing works
Self-citationParé, D. M., Lang, C., & Morris, M. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad74fe · Cited by 5 · see citing works
Star Formation in the Galactic Center
Kauffmann, J. (2016) · Proceedings of the International Astronomical Union · doi:10.1017/s1743921316012205 · Cited by 4 · see citing works
“The diffuse ionized gas is pervaded by a strong magnetic field ∼ 103 μG (Yusef-Zadeh et al. 1984; Uchida et al. 1985; Chuss et al. 2003; Novak et al. 2003) that also penetrates the CMZ clouds (Pillai et al. 2015).”
BackgroundNonsteady MHD Jets from Magnetized Accretion Disks — Sweeping-Magnetic-Twist Mechanism —
Shibata, K., & Uchida, Y. (1989) · Springer eBooks · doi:10.1007/978-94-009-1037-9_7 · Cited by 4 · see citing works
Self-citationMHD Mechanisms for the Formation of Galactic Center Lobes
Shibata, K. (1989) · Springer eBooks · doi:10.1007/978-94-009-2362-1_40 · Cited by 4 · see citing works
Self-citationLow-frequency Absorption and Radio Recombination Line Features of the Galactic Center Lobe
Hurley-Walker, N., Anderson, L. D., Luisi, M., McClure-Griffiths, N., Benjamin, R. A., Kuhn, M., Linville, D. J., Liu, B., & Zucker, C. (2024) · Astrophysical Journal · doi:10.3847/1538-4357/ad4d92 · Cited by 2 · see citing works
“Multiple authors have suggested that the GCL is created by activity in the Galactic center, either due to Sgr A ∗ (e.g., Uchida et al. 1985; Kassim et al. 1986) or due to star formation in the Central Molecular Zone (e.g. Law et al. 2009).”
BackgroundThe Galactic Center Lobe as an H ii Region
Anderson, L. D., Luisi, M., Liu, B., Linville, D. J., Benjamin, R. A., Hurley-Walker, N., McClure‐Griffiths, N. M., & Zucker, C. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad4d93 · Cited by 3 · see citing works
“…Law (2010) estimated that three large star clusters in the Galactic center region could account for the ionization of the GCL. Multiple studies have explored the idea that the GCL re-sults from twisting of poloidal magnetic field lines by Galactic rotation (Sofue 1985; Uchida et al. 1985, 1990).”
BackgroundGlobal Structure of Magnetic Fields in Spiral Galaxies
Sofue, Y. (1987) · Springer eBooks · doi:10.1007/978-3-642-72621-7_5 · Cited by 3 · see citing works
Self-citationMapping Magnetic Fields in the Cold Dust at the Galactic Center
Chuss, D. T., Novak, G., Davidson, J. A., Dotson, J., Dowell, C. D., Hildebrand, R. H., & Vaillancourt, J. E. (2003) · Astronomische Nachrichten · doi:10.1002/asna.200385099 · Cited by 2 · see citing works
“Uchida et al. (1985) have constructed a model that connects poloidal and toroidal fields.”
Wakefield Acceleration in a Jet from a Neutrino-driven Accretion Flow around a Black Hole
Kato, Y., Ebisuzaki, T., & Tajima, T. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac56e3 · Cited by 2 · see citing works
“The pioneering MHD simulations of magnetically driven jets from accretion disks were performed by Uchida et al. (1985) Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.”
MethodInfluentialLarge-Scale Ejection Structures in the Galactic Center
Sofue, Y. (1989) · Symposium - International Astronomical Union · doi:10.1017/s0074180900186565 · Cited by 2 · see citing works
Self-citationObservation of Toroidal Magnetic Fields on 100 pc Scales in the Galactic Center
Novak, G., Chuss, D. T., Dotson, J., Griffin, G. S., Loewenstein, R. F., Newcomb, M., Pernic, D., Peterson, J. B., & Renbarger, T. (2003) · Astronomische Nachrichten · doi:10.1002/asna.200385078 · Cited by 1 · see citing works
“In the model of Uchida et al. (1985), the GCL represents a gas outflow that is magnetically driven.”
BackgroundResultInfluentialEvidence for a Mass Outflow from Our Galactic Center
Law, C. J. (2007) · Proceedings of the International Astronomical Union · doi:10.1017/s1743921308020760 · Cited by 1 · see citing works
“• A magnetodynamic effect (Uchida et al. 1985, Shibata & Uchida 1987) —”
BackgroundPostwar Development of Astrophysics, 1946–2000 (Part II: Astrophysics)
Kogure, T. (2021) · Historical & cultural astronomy · doi:10.1007/978-3-030-57061-3_7 · Cited by 1 · see citing works
Three-Dimensional MHD Simulations of Accretion Disks and Jet Formation
Matsumoto, R., Matsuzaki, T., Tajima, T., & Shibata, K. (2001) · Astrophysics and space science library · doi:10.1007/978-94-010-0864-8_29 · Cited by 1 · see citing works
Self-citationThe Galactic Center Nonthermal Filaments: Recent Observations and Theory
LaRosa, T. N., Nord, M. E., Lazio, T. J. W., Shore, S. N., & Kassim, N. E. (2003) · Astronomische Nachrichten · doi:10.1002/asna.200385066 · Cited by 1 · see citing works
Mapping Magnetic Fields in the Cold Dust at the Galactic Center
Chuss, D. T., Novak, G., Davidson, J. A., Dotson, J., Dowell, C. D., Hildebrand, R. H., & Vaillancourt, J. E. (2003) · doi:10.1002/9783527617982.ch26 · Cited by 1 · see citing works
MHD Models of Galactic Center Lobes, Shells, and Filaments
Shibata, K., & Matsumoto, R. (1990) · Springer eBooks · doi:10.1007/978-94-009-0569-6_120 · Cited by 1 · see citing works
Self-citationJets from Magnetized Accretion Disks
Matsumoto, R. (2011) · Geophysical monograph · doi:10.1029/gm111p0293
MHD Models of Galactic Center Lobes, Shells, and Filaments
Shibata, K., & Matsumoto, R. (1990) · Symposium - International Astronomical Union · doi:10.1017/s0074180900190564
Self-citationShibata, K. (1990) · Symposium - International Astronomical Union · doi:10.1017/s0074180900190680
Self-citationStark, A. A. (2011) · Smithsonian Institution Scholarly Press eBooks · doi:10.5479/si.9781935623069.197
“The data show that all of the existing observations of large-scale magnetic fields in the Galactic Center are basically consistent with the “magnetic outflow” model of Uchida et al. (1985).”
ResultRadio continuum and molecular gas in the Galactic Center
Sofue, Y. (2007) · Springer eBooks · doi:10.1007/bfb0101978
“An MHD acceleration model in which the gas is accelerated by a twist of poloidal magnetic field by an accreting gas disk has been proposed (Uchida et al 1985; Uchida and Shibata 1986).”
BackgroundMethodSelf-citationSweeping-Magnetic-Twist Mechanism and Molecular Bipolar Flows
Shibata, K., & Uchida, Y. (1987) · Symposium - International Astronomical Union · doi:10.1017/s0074180900096029
Self-citationThe galactic center-radio continuum study
Sofue, Y. (1988) · Vistas in Astronomy · doi:10.1016/0083-6656(88)90205-x
Self-citationParticle energization in galactic centre ejections
Jansen, F. A., & Kirchner, T. M. (1991) · Astrophysics and Space Science · doi:10.1007/bf00646945
4.1. Radio continuum and molecular gas in the Galactic center: large-scale structures
Sofue, Y. (1998) · Symposium - International Astronomical Union · doi:10.1017/s0074180900084473
Self-citationObservation of Toroidal Magnetic Fields on 100 pc Scales in the Galactic Center
Novak, G., Chuss, D. T., Dotson, J., Griffin, G. S., Loewenstein, R. F., Newcomb, M., Pernic, D., Peterson, J. B., & Renbarger, T. (2003) · doi:10.1002/9783527617982.ch19
Shibata, K. (1990) · Springer eBooks · doi:10.1007/978-94-009-0569-6_132
Self-citationThe Galactic Center Nonthermal Filaments: Recent Observations and Theory
LaRosa, T. N., Nord, M. E., Joseph, T., Lazio, W., Shore, S. N., & Kassim, N. E. (2003) · doi:10.1002/9783527617982.ch27
MHD Mechanisms for the Formation of Galactic Center Lobes
Shibata, K. (1989) · Symposium - International Astronomical Union · doi:10.1017/s007418090018667x
Self-citationMHD Aspects of Galactic Center Physics
Heyvaerts, J. F. (1989) · Symposium - International Astronomical Union · doi:10.1017/s0074180900186668
Sweeping-Magnetic-Twist Mechanism and Molecular Bipolar Flows
Shibata, K., & Uchida, Y. (1987) · Springer eBooks · doi:10.1007/978-94-009-4782-5_127
Self-citationMHD Aspects of Galactic Center Physics
Heyvaerts, J. F. (1989) · Springer eBooks · doi:10.1007/978-94-009-2362-1_39
The Magnetic Field in the Inner 70 Parsecs of the Milky Way
Morris, M. (1990) · Symposium - International Astronomical Union · doi:10.1017/s0074180900190515
SDSS-V LVM: Verifying what, and where, the “Galactic center lobe” is
Kreckel, K., Egorov, O. V., Drory, N., Blanc, G. A., Méndez-Delgado, J. E., Kabanovic, S., Bizyaev, D., Brownstein, J. R., Egorova, E., Fernández-Trincado, J. G., et al. (2026) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202659505
- Authors
- Uchida, Y., Shibata, K., & Sofue, Y.
- Affiliations
- The University of Tokyo (JP)
- Aichi University of Education (JP)
- Venue
- Nature
- Published
- 1985-10
- Volume
- 317
- Issue
- 6039
- Pages
- 699-701
- ISSN
- 0028-0836 (ISSN-L)
- 1476-4687
- OpenAlex
- W2070225683
- Cited by
- 72
- References
- 14
- Citations by year
- 2026: 1 · 2024: 5 · 2022: 1 · 2021: 1 · 2019: 3 · 2018: 1 · 2017: 5 · 2016: 2 · 2015: 1 · 2014: 1 · 2013: 1
- FWCI
- 2.56
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Nature (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Astrophysics and Cosmic Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- Milky Way, radio lobes, magnetic twist, radio continuum emission
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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