The geometry of the magnetic field in the central molecular zone measured by PILOT

A. Mangilli; J. Aumont; J.-Ph. Bernard; A. Buzzelli; G. de Gasperis; J. B. Durrive; K. Ferriere; G. Foënard; A. Hughes; A. Lacourt; R. Misawa; L. Montier; B. Mot; I. Ristorcelli; H. Roussel; P. Ade; D. Alina; P. de Bernardis; E. de Gouveia Dal Pino; J. P. Dubois; C. Engel; V. Guillet; P. Hargrave; R. Laureijs; Y. Longval; B. Maffei; A. M. Magalhes; C. Marty; S. Masi; J. Montel; F. Pajot; E. Pérot; L. Rodriguez; M. Salatino; M. Saccoccio; G. Savini; S. Stever; J. Tauber; C. Tibbs; C. Tucker

doi:10.1051/0004-6361/201935072

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Volume 630 (October 2019)

A&A, 630 (2019) A74

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Table 1

Magnetic field strength estimates for CMZ clouds, assuming equipartition between magnetic pressure and ram pressure (see text in Sect. 5.3).

Cloud		δv_LOS	B_equ
	(cm⁻³)	(km s⁻¹)	(mG)
Sgr B2	5.0	20	3.9–5.8
50 km s⁻¹	4.5	10	0.3–1.7
20 km s⁻¹	4.3	10	0.5–1.2
Brick	4.2	5	0.2–0.5

Notes. The range of values quoted for B_equ corresponds to varying the angle between B and the LOS in the range 0° < ζ < 90°.

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