2013ApJ...767...33E


Query : 2013ApJ...767...33E

2013ApJ...767...33E - Astrophys. J., 767, 33 (2013/April-2)

A mathematical model for an hourglass magnetic field.

EWERTOWSKI B. and BASU S.

Abstract (from CDS):

Starting with a mathematical boundary value problem for the magnetic vector potential in an axisymmetric cylindrical coordinate system, we derive a general solution for any arbitrary current distribution using the method of Green's functions. We use this to derive an analytic form for an hourglass magnetic field pattern created by electrical currents that are concentrated near (but not confined within) the equatorial plane of a cylindrical coordinate system. Our solution is not characterized by a cusp at the equatorial plane, as in previous solutions based on a current sheet. The pattern we derive provides a very good fit to hourglass magnetic field patterns emerging from three-dimensional numerical simulations of core formation, and can in principle be used for source-fitting of observed magnetic hourglass patterns.

Abstract Copyright:

Journal keyword(s): ISM: individual (NGC 1333 IRAS 4A, G31.41+0.31) - ISM: magnetic fields - methods: analytical - stars: formation

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 [JCC87] IRAS 4A Y*O 03 29 10.49 +31 13 30.8           ~ 715 1
2 [JCC87] IRAS 4 FIR 03 29 10.9 +31 13 26           ~ 478 0
3 [JCC87] IRAS 4B Y*O 03 29 12.058 +31 13 02.05           ~ 600 0
4 IRAS 18449-0115 cor 18 47 34.27 -01 12 43.2           ~ 388 0

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