2018MNRAS.474.5330E


Query : 2018MNRAS.474.5330E

2018MNRAS.474.5330E - Mon. Not. R. Astron. Soc., 474, 5330-5339 (2018/March-2)

The Stormer problem for an aligned rotator.

EPP V. and PERVUKHINA O.N.

Abstract (from CDS):

The effective potential energy of the particles in the field of rotating uniformly magnetized celestial body is investigated. The axis of rotation coincides with the axis of the magnetic field. Electromagnetic field of the body is composed of a dipole magnetic and quadrupole electric fields. The geometry of the trapping regions is studied as a function of the magnetic field magnitude and the rotation speed of the body. Examples of the potential energy topology for different values of these parameters are given. The main difference from the classical Stormer problem is that the single toroidal trapping region predicted by Stormer is divided into equatorial and off-equatorial trapping regions. Applicability of the idealized model of a rotating uniformly magnetized sphere with a vacuum magnetosphere to real celestial bodies is discussed.

Abstract Copyright: © 2017 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): astroparticle physics - dynamo - relativistic processes - methods: analytical - planets and satellites: aurorae - stars: rotation

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 LSR J1835+3259 PM* 18 35 37.8801226673 +32 59 53.316099140   20.0   17.1   M8.5V 160 0

Query : 2018MNRAS.474.5330E

Basic data :
LSR J1835+3259 -- High Proper Motion Star
Other object types:
otypes_help
* (CNS5,Karmn,...), PM* (2007AJ,LSPM,...), Rad (2006ApJ,[B2006]), BD* (2023Sci), NIR (2MASS), MIR (WISEA), IR (2MASSI)
ICRS coord. (ep=J2000) :
18 35 37.8801226673 +32 59 53.316099140 (Optical) [ 0.0360 0.0423 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
18 33 47.2573357140 +32 57 59.840667707 [ 0.0360 0.0423 90 ]
Gal coord. (ep=J2000) :
061.6459615099674 +17.4440026082828 [ 0.0360 0.0423 90 ]
Proper motions mas/yr :
-72.650 -755.146 [0.047 0.052 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) 8.4 [2.0] / z(~) 0.000028 [0.000007] / cz 8.40 [2.00]
   (NIR) B 2012AJ....144...99D
Parallaxes (mas):
175.7930 [0.0468] A 2020yCat.1350....0G
Spectral type:
M8.5V C 2012AJ....144...99D
Fluxes (6) :
B 20.0 [~] E 2003AJ....125..984M
R 17.1 [~] E 2003AJ....125..984M
G 14.850962 [0.002895] C 2020yCat.1350....0G
J 10.270 [0.022] C 2003yCat.2246....0C
H 9.617 [0.021] C 2003yCat.2246....0C
K 9.171 [0.018] C 2003yCat.2246....0C
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Identifiers (13) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

2MASS J18353790+3259545 LSR J1835+3259 USNO-B1.0 1229-00376318 Gaia DR2 2091177593123254016
CNS5 4601 2MASSI J1835379+325954 WISEA J183537.82+325945.4
Karmn J18356+329 2MUCD 11792 [B2006] J183537.9+325955
LSPM J1835+3259 TIC 27858644 Gaia DR3 2091177593123254016

References (160 between 1850 and 2026) (Total 160)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 4    Distance : 6    Var : 3    Rot : 2    Fe/H : 2    Plx : 4    PM : 6    SpT : 5   

   


External archives :

Link by name to the catalogue in VizieR :

2MASS J18353790+3259545 LSPM J1835+3259 2MASSI J1835379+325954 USNO-B1.0 1229-00376318 WISEA J183537.82+325945.4
Gaia DR3 2091177593123254016 Gaia DR2 2091177593123254016

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