REVIEW 3 major objections 5 minor 73 references
Radio filaments as Z-pinched Galactic center wind
T0 review · 3 major / 5 minor · reviewed 2026-08-11 · deepseek-v4-flash
Pith's one-line read The paper proposes that the nonthermal radio filaments at the Galactic center are produced when the Galactic center wind blows across magnetic structures, creating a current that Z-pinches into filaments and accelerates electrons to…
desk verdict A well-framed, honestly tentative proposal for Galactic center radio filaments; the uncalculated current-generation step is the main soft spot, but the idea is novel and deserves refereeing. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The load-bearing machinery is the Z-pinch: a current-carrying plasma column in which the self-generated azimuthal magnetic field exerts a compressive (pinching) force, described quantitatively by the generalized Bennett relation. The paper applies this relation to a current of ~$10^{15}$–$10^{16}$ A set up by the wind's differential deflection of electrons and ions, deriving from it the pinching pressure, a pinching timescale of ~$10^{2}$–$10^{3}$ yr, and the axial electric field needed to accelerate electrons; it then invokes the diocotron instability — a plasma instability in which shear in the electron flow converts radial charge separation into azimuthal vortical motion — as the channel by which an axial magnetic field is generated to stabilize the column. The central identity is Eq. (2), I[A] ≈ (3 × $10^{12}$) × 2πa[pc] Bf_z[G]/µ0, which ties the observed filament width and axial field to the current that drives the whole process.
What would settle it
A particle-in-cell or magnetohydrodynamic simulation of a Galactic center-like wind (density $10^{-2}$–$10^{-1}$ $cm^{-3}$, speed $10^{5}$–$10^{6}$ m/s) flowing past a magnetic structure of 10 µG–100 mG would settle whether the claimed net axial current of $10^{15}$–$10^{16}$ A is actually established before return currents and field-line closure cancel it. Observationally, the model's low-Lorentz-factor variant predicts that some high-latitude filaments should be brighter at ultra-long radio wavelengths than standard higher-gamma models suggest; a sensitive low-frequency survey of the Galactic center could test this.
Extended reading notes
Core claim
The central claim is that the Galactic center's nonthermal radio filaments are the product of a Z-pinch operating on the Galactic center wind. The wind carries a partially ionized plasma outward from the plane; when it encounters local magnetic structures (molecular clouds, HII regions, or field inhomogeneities), the electrons and ions, having opposite charges and very different masses, are deflected unequally and a net axial current is set up. That current, of order $10^{15}$–$10^{16}$ A, creates an azimuthal magnetic field that pinches the plasma into long filaments. Because the magnetic field must rearrange during the constriction, a toroidal displacement current appears, which by Maxwell's equations requires a poloidal electric field along the filament; this field accelerates runaway electrons to Lorentz factors of order 100 or more, and the ensuing synchrotron radiation is the observed nonthermal radio emission. The same process generates an axial magnetic field — most plausibly via the diocotron instability — that halts the pinch and stabilizes the filament against kink and sausage modes, accounting for the predominantly axial field orientation and the observed braided fine structure.
Load-bearing premise
The entire chain depends on the premise that the wind's passage over local magnetic structures actually produces a net axial current of order $10^{15}$–$10^{16}$ A that is not canceled by return currents; the paper itself concedes that 'cancellations are likely as the field needs to close up into loops' and states it cannot give a detailed quantitative analysis of the deflection process.
Editorial extensions
If this is right
- The filaments' orientation perpendicular to the plane is set by the wind direction, not by a global poloidal magnetic field, removing the need for a highly ordered 'backbone' field at the Galactic center.
- The observed predominantly axial magnetic field in filaments is a natural steady-state outcome: the axial field grows until it balances the pinching pressure, and must exceed the azimuthal component by roughly an order of magnitude to suppress kink and sausage instabilities.
- The model accounts for the observed spread and sign changes in filament spectral indices: where the synchrotron peak sits relative to the observing band varies naturally, and because electrons are accelerated progressively along the filament, spectral index should trend monotonically with Galactic latitude.
- The required electron Lorentz factors can be as low as ~100, so some filaments may peak at frequencies below the usual GHz windows; future ultra-long-wavelength observations could catch this.
- Young, dimmer filaments in their formative stage should be detectable by upcoming more sensitive instruments, offering a direct way to watch the pinch develop.
Reading between the lines
- If the Z-pinch mechanism is generic, similar wind-driven radio filaments should appear in other galactic nuclei with strong outflows and dense magnetic structures; targeted searches in nearby starburst or Seyfert galaxies could test this prediction.
- The paper's assumption that the net current survives return-current cancellation is the crux; a more rigorous treatment of field-line closure and the Hall effect in the wind–structure interaction would either confirm or kill the model, and could be done with existing plasma simulation codes.
- The model effectively turns radio filaments into probes of the Galactic center wind: measuring the variation of spectral index along a filament could map the wind speed and local magnetic structure, an observational program not discussed explicitly in the paper.
- Because the paper works in SI units and order-of-magnitude estimates, the same set of relations could be cross-checked against laboratory Z-pinch experiments scaled to astrophysical parameters, providing an empirical anchor for the claimed stabilizing role of the axial field.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper proposes that the nonthermal radio filaments in the Galactic center are formed when the Galactic center wind washes over magnetic field structures: the disparate charge-to-mass ratios of electrons and ions lead to a current, which is Z-pinched into filaments; the time-varying azimuthal magnetic field induces an axial electric field that accelerates electrons to relativistic energies, producing synchrotron emission; a self-generated axial magnetic field, possibly via the diocotron instability, stabilizes the filaments. The paper presents order-of-magnitude estimates for the pinch current, the required accelerating field, and the stabilizing field, comparing them to observed filament properties.
Significance. If the mechanism were correct, it would offer a self-consistent scenario in which the axial magnetic field of the filaments is generated locally rather than inherited from an ordered background poloidal field, which is attractive given observations that do not show a dominant poloidal field outside the filaments. The paper gives a clear chain of plasma-physics estimates and makes falsifiable predictions, such as spectral-index trends with Galactic latitude and possible ultra-long-wavelength emission. However, the central premise—that the wind can sustain a net axial current of ~1e15–1e16 A—is not derived; the paper explicitly concedes that cancellations are likely and that no detailed quantitative analysis is attempted. Moreover, the basic charge-separation picture is inconsistent with the expected dynamics of a collisionless magnetized plasma, and the quantitative links are largely circular. The manuscript is an honest speculation, but the load-bearing first step remains unsupported.
major comments (3)
- [II A] The pinch current I is not derived from the wind–magnetic-field interaction; it is inferred from the observed axial field Bf_z via the Bennett relation (Eq. 2). All subsequent quantities—Bφ in Eq. (17), E in Eq. (14), and Bz in Eq. (22)—scale with I, so the entire mechanism rests on this inferred value. The paper admits 'cancellations are likely as the field needs to close up into loops' and states it is 'unable to attempt a detailed quantitative analysis.' Without a concrete calculation showing that a net axial current of this magnitude is generated and that return currents do not cancel it, the proposed Z-pinch chain does not begin.
- [I, item A; II A] The charge-separation mechanism is physically problematic. In a collisionless magnetized plasma, the E×B drift is charge- and mass-independent, so the stated 'bulk velocity differential' cannot be sustained by the Lorentz force alone. The polarization drift does separate charges, but it is transient and is quenched by the induced space-charge electric field. The paper does not explain what maintains a net current along the filament axis, and its claim that 'whatever the magnetic field configuration' electrons are more strongly deflected is not valid in the magnetized, force-free regime the paper itself invokes in Sec. II C.
- [II C] The claimed consistency between the terminal axial field from the diocotron estimate (Eq. 22) and the observed Bf_z is a circular test, because the current I in Eq. (22) was set by the same observed Bf_z through Eq. (2). The agreement is therefore a self-consistency check rather than an independent prediction; this should be stated clearly, and the text should avoid presenting it as confirmation.
minor comments (5)
- [II A, Eq. (3)] The relation between I and Δv⊥ is not shown. If I = n e Δv⊥ (π a²), the quoted range of 10⁻⁴–10⁻² m/s is plausible for the stated parameters, but the intermediate expression should be given.
- [II A, Eq. (2)] The numerical factor '3 × 10¹²' combined with μ0 in the denominator is dimensionally confusing; please specify the unit system or provide the conversion explicitly.
- [II B] The symbol E_min is used for both the electric field (Eq. 14) and an energy (Eq. 21); please use different symbols to avoid ambiguity.
- [II B] The sentence 'Compare E_min with Eqs. 7 through 10 of [26]' is unclear because the content of those equations is not reproduced; please spell out the comparison.
- [II B] The sign convention for the axial electric field and the direction of electron acceleration relative to the Galactic plane should be clarified, as the text says electrons are accelerated toward the plane while the electric field points away from it.
Circularity Check
No significant circularity: the current is inferred from the observed axial field as a consistency check, not predicted from it and then relabeled as an independent forecast.
full rationale
The paper is an explicitly tentative, order-of-magnitude proposal. Its central premise—that the Galactic-center wind creates a net axial current of ~1e15–1e16 A via charge separation—is not derived from first principles; the paper instead infers the current required by the observed axial field through the Bennett relation (Eq. 2), and then tests whether that current is consistent with the other parts of the mechanism (Ampère-law azimuthal field, inductive electric field, runaway threshold, and diocotron threshold). This is a self-consistency check, not a circular derivation: the current is a model parameter set by one observed quantity, and the subsequent equations are independent relations involving that parameter. The later comparison of the diocotron terminal field with the observed Bf_z is partially inherited, because I in Eq. (22) was fixed by Eq. (2) using the same Bf_z; however, the diocotron relation also contains independent inputs (Vmin from the electron-acceleration requirement, L, a), and the resulting coefficient is not identically unity, so the comparison retains some falsifiable content. The paper explicitly concedes the main gap: "cancellations are likely as the field needs to close up into loops" and "we are unable to attempt a detailed quantitative analysis of the deflection process post-haste." That is an unverified assumption, which is a scientific-correctness risk, not a circularity. There are no load-bearing self-citations: the plasma formulae are drawn from external references (Peratt, Bennett, Witalis, etc.), and no unique result is imported from the author's own prior work. I therefore find no step in the derivation that reduces, by construction or by self-citation, to its own input.
Assumptions & free parameters
free parameters (8)
- Bf_z (observed axial field along filaments) =
0.1 to 1 mG
- n_e = n_i (plasma density) =
0.01 to 0.1 cm^-3
- T (wind temperature) =
about 100 K
- B_struct (local magnetic structure strength) =
10 microG to 100 mG
- v_wind =
1e5 to 1e6 m/s
- a (filament width) =
about 0.5 pc
- L and w (filament length and pre-pinching width) =
L about 100 pc, w about 10 pc
- zeta (runaway electron fraction) =
order unity
assumptions (5)
- domain assumption Generalized Bennett relation describes force balance in the filament
- domain assumption Z-pinch stability criteria (Suydam, kink, sausage) apply to the filament
- domain assumption Diocotron instability formula gives the e-folding length and the generated Bz
- domain assumption The plasma is collisionless and magnetically dominated so that ideal, force-free MHD applies
- ad hoc to paper A net axial current survives despite loop-closing field geometry
Cite this review
Pith. "Pith review of Radio filaments as Z-pinched Galactic center wind." pith.science (2026). https://pith.science/paper/M3QXQKVN
@misc{pith2026241215575,
author = {Pith},
title = {Pith review of: Radio filaments as Z-pinched Galactic center wind},
year = {2026},
howpublished = {\url{https://pith.science/paper/M3QXQKVN}},
note = {Machine review of arXiv:2412.15575}
}
read the original abstract
In this brief note, we tentatively investigate the possibility that the radio filaments are produced when the Galactic center wind washes over magnetic field structures. The electrons and ions, with their disparate charge-to-mass ratios, are deflected differently by the magnetic field, and a current results. The current is subsequently Z-pinched into filaments, creating an electron-accelerating electric field along the way, because the magnetic field necessarily rearranges during the dynamic constriction process. An axial magnetic field also arises, possibly via the diocotron channel, to eventually quench the pinching and stabilize the filaments against a variety of instabilities.
Reference graph
Works this paper leans on
-
[1]
F. Yusef-Zadeh, R. G. Arendt, M. Wardle, and I. Hey- wood, The Astrophysical Journal Letters 949, L31 (2023), 2306.01071
work page Pith review arXiv 2023
- [2]
-
[3]
H. S. Liszt, The Astrophysical Journal Letters 293, L65 (1985)
work page 1985
-
[4]
F. Yusef-Zadeh, M. Morris, O. B. Slee, and G. J. Nelson, The Astrophysical Journal 310, 689 (1986)
work page 1986
-
[5]
A. D. Gray, L. E. Cram, R. D. Ekers, and W. M. Goss, Nature 353, 237 (1991)
work page 1991
-
[6]
R. F. Haynes, R. T. Stewart, A. D. Gray, W. Reich, P. Re- ich, and U. Mebold, Astronomy & Astrophysics 264, 500 (1992)
work page 1992
-
[7]
C. C. Lang, M. Morris, and L. Echevarria, The Astrophys- ical Journal 526, 727 (1999), astro-ph/9906336
arXiv 1999
- [8]
Show all 73 references
-
[9]
Yusef-Zadeh, J
F. Yusef-Zadeh, J. W. Hewitt, and W. Cotton, The Astro- physical Journal Supplement Series 155, 421 (2004), astro- ph/0409292
2004
-
[10]
C. J. Law, F. Yusef-Zadeh, and W. D. Cotton, The As- trophysical Journal Supplement Series 177, 515 (2008), 0803.1412
2008 arXiv
-
[11]
Yusef-Zadeh, R
F. Yusef-Zadeh, R. G. Arendt, M. Wardle, I. Heywood, W. Cotton, and F. Camilo, The Astrophysical Journal Let- ters 925, L18 (2022), 2201.10552
2022 arXiv
-
[12]
Yusef-Zadeh, R
F. Yusef-Zadeh, R. G. Arendt, M. Wardle, S. Boldyrev, I. Heywood, W. Cotton, and F. Camilo, Monthly No- tices of the Royal Astronomical Society 515, 3059 (2022), 2206.10732
2022 arXiv
-
[13]
Yusef-Zadeh, R
F. Yusef-Zadeh, R. G. Arendt, M. Wardle, I. Heywood, and W. Cotton, Monthly Notices of the Royal Astronomical So- ciety 517, 294 (2022), 2208.11589
2022 arXiv
-
[14]
Yusef-Zadeh, R
F. Yusef-Zadeh, R. G. Arendt, and M. Wardle, The Astro- physical Journal Letters 939, L21 (2022), 2210.04913
2022 arXiv
-
[15]
Lesch and W
H. Lesch and W. Reich, Astronomy and Astrophysics 264, 493 (1992)
1992
-
[16]
Rosner and G
R. Rosner and G. Bodo, The Astrophysical Journal Letter s 470, L49 (1996)
1996
-
[17]
Nicholls and E
J. Nicholls and E. T. Le Strange, The Astrophysical Jour nal 443, 638 (1995)
1995
-
[18]
S. N. Shore and T. N. LaRosa, Astrophysical Journal 521, 587 (1999), astro-ph/9904048
1999 arXiv
-
[19]
G. V. Bicknell and J. Li, The Astrophysical Journal Lett ers 548, L69 (2001), astro-ph/0011382
2001 arXiv
-
[20]
R. B. Dahlburg, G. Einaudi, T. N. LaRosa, and S. N. Shore, The Astrophysical Journal 568, 220 (2002), astro- ph/0112378
2002
-
[21]
Yusef-Zadeh, The Astrophysical Journal 598, 325 (2003), astro-ph/0308008
F. Yusef-Zadeh, The Astrophysical Journal 598, 325 (2003), astro-ph/0308008
2003 arXiv
-
[22]
Boldyrev and F
S. Boldyrev and F. Yusef-Zadeh, The Astrophysical Jour nal Letters 637, L101 (2006), astro-ph/0512373
2006 arXiv
-
[23]
Linden, D
T. Linden, D. Hooper, and F. Yusef-Zadeh, Astrophysica l Journal 741, 95 (2011), 1106.5493
2011 arXiv
-
[24]
W. E. Banda-Barrag´ an, E. R. Parkin, C. Federrath, R. M. Crocker, and G. V. Bicknell, Monthly Notices of the Royal Astronomical Society 455, 1309 (2016), 1510.05356
2016 arXiv
-
[25]
Yusef-Zadeh and M
F. Yusef-Zadeh and M. Wardle, Monthly Notices of the Royal Astronomical Society 490, L1 (2019), 1909.07409
2019 arXiv
-
[26]
Thomas, C
T. Thomas, C. Pfrommer, and T. Enßlin, The Astrophysica l Journal Letters 890, L18 (2020), 1912.08491
2020 arXiv
-
[27]
Sofue, Publications of the Astronomical Society of J apan 72, L4 (2020), 2001.11827
Y. Sofue, Publications of the Astronomical Society of J apan 72, L4 (2020), 2001.11827
2020 arXiv
-
[28]
E. R. Coughlin, C. J. Nixon, and A. Ginsburg, Monthly Notices of the Royal Astronomical Society 501, 1868 (2021), 2010.13790
2021 arXiv
-
[29]
Sofue, Monthly Notices of the Royal Astronomical Soc i- ety 518, 6273 (2023), 2210.17219
Y. Sofue, Monthly Notices of the Royal Astronomical Soc i- ety 518, 6273 (2023), 2210.17219
2023 arXiv
-
[30]
Gregori, F
G. Gregori, F. Miniati, D. Ryu, and T. W. Jones, The As- trophysical Journal 543, 775 (2000)
2000
-
[31]
R. M. Crocker, D. I. Jones, F. Aharonian, C. J. Law, F. Melia, and J. Ott, Monthly Notices of the Royal As- tronomical Society 411, L11 (2011), 1009.4340
2011 arXiv
-
[32]
Yusef-Zadeh, J
F. Yusef-Zadeh, J. W. Hewitt, M. Wardle, V. Tatischeff, D. A. Roberts, W. Cotton, H. Uchiyama, M. Nobukawa, T. G. Tsuru, C. Heinke, et al., The Astrophysical Journal 762, 33 (2013), 1206.6882
2013 arXiv
-
[33]
T. Oka, T. R. Geballe, M. Goto, T. Usuda, Benjamin, J. McCall, and N. Indriolo, The Astrophysical Journal 883, 54 (2019), 1910.04762
2019
-
[34]
Le Petit, M
F. Le Petit, M. Ruaud, E. Bron, B. Godard, E. Roueff, D. Languignon, and J. Le Bourlot, Astronomy & Astro- physics 585, A105 (2016), 1510.02221
2016 arXiv
-
[35]
M. G. Haines, Plasma Physics and Con- trolled Fusion 53, 093001 (2011), URL https://dx.doi.org/10.1088/0741-3335/53/9/093001
2011 doi
-
[36]
W. H. Bennett, Physical Review 45, 890 (1934)
1934
-
[37]
A. L. Peratt, Physics of the Plasma Universe (2015)
2015
-
[38]
Carlqvist and G
P. Carlqvist and G. F. Gahm, IEEE Transactions on Plasma Science 20, 867 (1992)
1992
-
[39]
Benford, The Astrophysical Journal 333, 735 (1988)
G. Benford, The Astrophysical Journal 333, 735 (1988)
1988
-
[40]
B. A. Trubnikov, Soviet Physics Uspekhi 33, 1061 (1990), URL https://dx.doi.org/10.1070/PU1990v033n12ABEH002667
1990 doi
-
[41]
Par´ e, N
D. Par´ e, N. O. Butterfield, D. T. Chuss, J. A. Guerra, J. I . Iuliano, K. Karpovich, M. R. Morris, and E. J. Wollack, The Astrophysical Journal 969, 150 (2024), 2401.05317
2024 arXiv
-
[42]
Nishiyama, H
S. Nishiyama, H. Hatano, M. Tamura, N. Matsunaga, T. Yoshikawa, T. Suenaga, J. H. Hough, K. Sugitani, T. Na- gayama, D. Kato, et al., The Astrophysical Journal Letters 722, L23 (2010), 1009.0584
2010 arXiv
-
[43]
D. M. Par´ e, C. C. Lang, M. R. Morris, H. Moore, and S. A. Mao, The Astrophysical Journal 884, 170 (2019), 1909.08268
2019 arXiv
-
[44]
E. A. Witalis, Physical Review A 24, 2758 (1981)
1981
-
[45]
Carlqvist, Astrophysics and Space Science 144, 73 (1988)
P. Carlqvist, Astrophysics and Space Science 144, 73 (1988)
1988
-
[46]
Takakura, Publications of the Astro- nomical Society of Japan 12 (1960), URL https://api.semanticscholar.org/CorpusID:118389204
T. Takakura, Publications of the Astro- nomical Society of Japan 12 (1960), URL https://api.semanticscholar.org/CorpusID:118389204
1960
-
[47]
aki Kawabata, Publications of the Astro- nomical Society of Japan 16, 30 (1964), URL 7 https://api.semanticscholar.org/CorpusID:115780670
K. aki Kawabata, Publications of the Astro- nomical Society of Japan 16, 30 (1964), URL 7 https://api.semanticscholar.org/CorpusID:115780670
1964
-
[48]
Kai, Publications of the Astronomical Society of Jap an 17, 294 (1965)
K. Kai, Publications of the Astronomical Society of Jap an 17, 294 (1965)
1965
-
[49]
B. E. Meierovich, Physics Reports 104, 259 (1984)
1984
-
[50]
B. R. Suydam, Journal of Nu- clear Energy 7, 275 (1958), URL https://api.semanticscholar.org/CorpusID:121860252
1958
-
[51]
J. P. Freidberg, Reviews of Modern Physics 54, 801 (1982)
1982
-
[52]
B. A. Trubnikov, Soviet Physics Uspekhi 34, 1018 (1991)
1991
-
[53]
D. D. Ryutov, M. S. Derzon, and M. K. Matzen, Reviews of Modern Physics 72, 167 (2000)
2000
-
[54]
Inoue, T
M. Inoue, T. Takahashi, H. Tabara, T. Kato, and M. Tsuboi, Publications of the Astronomical Society of Japan 36, 633 (1984)
1984
-
[55]
Tsuboi, T
M. Tsuboi, T. Kawabata, T. Kasuga, T. Handa, and T. Kato, Publications of the Astronomical Society of Japan 47, 829 (1995)
1995
-
[56]
Yusef-Zadeh, M
F. Yusef-Zadeh, M. Wardle, and P. Parastaran, The Astro - physical Journal Letters 475, L119 (1997)
1997
-
[57]
D. M. Pare, C. C. Lang, and M. R. Morris, arXiv e-prints arXiv:2408.16745 (2024), 2408.16745
2024 arXiv
-
[58]
D. M. Par´ e, C. C. Lang, and M. R. Morris, The Astrophys- ical Journal 941, 123 (2022), 2209.08153
2022 arXiv
-
[59]
Ferri` ere, Astronomy & Astrophysics 505, 1183 (2009), 0908.2037
K. Ferri` ere, Astronomy & Astrophysics 505, 1183 (2009), 0908.2037
2009 arXiv
-
[60]
R. M. Crutcher, D. A. Roberts, T. H. Troland, and W. M. Goss, The Astrophysical Journal 515, 275 (1999)
1999
-
[61]
Heiles, Y
C. Heiles, Y. H. Chu, and T. H. Troland, The Astrophysica l Journal Letters 247, L77 (1981)
1981
-
[62]
Morris, arXiv e-prints astro-ph/0701050 (2007), as tro- ph/0701050
M. Morris, arXiv e-prints astro-ph/0701050 (2007), as tro- ph/0701050
2007 arXiv
-
[63]
Buneman, Physical Review 115, 503 (1959)
O. Buneman, Physical Review 115, 503 (1959)
1959
-
[64]
L. P. Block, A double layer review (1977)
1977
-
[65]
D. D. Ryutov, IEEE Transactions on Plasma Science 43, 2363 (2015)
2015
-
[66]
Gold, in NASA Special Publication, edited by W
T. Gold, in NASA Special Publication, edited by W. N. Hess (1964), vol. 50, p. 389
1964
-
[67]
Alfven, Cosmical electrodynamics (1950)
H. Alfven, Cosmical electrodynamics (1950)
1950
-
[68]
Shishlov, R
A. Shishlov, R. Baksht, A. Labetsky, V. Oreshkin, A. Rousskikh, A. Fedunin, S. Chaikovsky, V. Kokshenev, N. Kurmaev, and F. Fursov, IEEE Transactions on Plasma Science 30, 498 (2002)
2002
-
[69]
Grainge, B
K. Grainge, B. Alachkar, S. Amy, D. Barbosa, M. Bommi- neni, P. Boven, R. Braddock, J. Davis, P. Diwakar, V. Fran- cis, et al., Astronomy Reports 61, 288 (2017)
2017
-
[70]
Wang, Scientia Sinica Physica, Mechanica & Astronom - ica 44, 783 (2014)
N. Wang, Scientia Sinica Physica, Mechanica & Astronom - ica 44, 783 (2014)
2014
-
[71]
M. Xue, W. Zhu, X. Wu, R. Xu, and H. Wang, Re- search in Astronomy and Astrophysics 23, 095005 (2023), 2307.03422
2023 arXiv
-
[72]
X. Chen, J. Yan, Y. Xu, L. Deng, F. Wu, L. Wu, L. Zhou, X. Zhang, X. Zhu, Z. Yang, et al., Chinese Journal of Space Science 43, 43 (2023)
2023
-
[73]
J. Silk, I. Crawford, M. Elvis, and J. Zarnecki, Philoso phical Transactions of the Royal Society of London Series A 379, 20190560 (2021)
2021
Reviewed August 11, 2026 · model on record in the stance chip above.
Discussion (0). Continue with ORCID to comment.