2022MNRAS.514.4069J


Query : 2022MNRAS.514.4069J

2022MNRAS.514.4069J - Mon. Not. R. Astron. Soc., 514, 4069-4077 (2022/August-2)

Measuring lens dimensionality in extreme scattering events through wave optics.

JOW D.L. and PEN U.-L.

Abstract (from CDS):

Compact radio sources have been observed to undergo large, frequency-dependent changes in intensity due to lensing by structures in the interstellar medium, in so-called 'extreme scattering events' (ESEs). While the study of astrophysical plasma lensing has primarily focused on the geometric limit of optics, coherent radio sources such as pulsars exhibit wave effects when lensed. The additional phase information provided by interference effects in the wave regime may yield more information about the lens than could be obtained in the geometric regime. In this paper, we show that, using wave effects, one can potentially distinguish a one-dimensional lens (where 'one-dimensional' includes both highly elongated lenses, as well as perfectly axisymmetric lenses) from a fully two-dimensional lens, with minimal assumptions on the form of the lensing potential.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): waves - pulsars: general - radio continuum: ISM

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 PSR J1959+2048 Psr 19 59 36.7643141520 +20 48 14.896407996   21.08 20.16 19.53 18.79 G: 854 3

Query : 2022MNRAS.514.4069J

Basic data :
PSR J1959+2048 -- Pulsar
Other object types:
otypes_help
gam (1FGL,2FGL,...), Psr (2022ApJS,PSR), Pl? (2020ApJ), V* (V*), * (Gaia)
ICRS coord. (ep=J2000) :
19 59 36.7643141520 +20 48 14.896407996 (Optical) [ 0.6353 0.7032 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
19 57 25.0391949060 +20 40 00.756655463 [ 0.6353 0.7032 90 ]
Gal coord. (ep=J2000) :
059.1968896728793 -04.6974899421032 [ 0.6353 0.7032 90 ]
Proper motions mas/yr :
-19.267 -26.560 [1.235 1.244 90] A 2020yCat.1350....0G
Parallaxes (mas):
1.1878 [1.3556] A 2020yCat.1350....0G
Spectral type:
G: E 1992ApJ...400..638A
Fluxes (6) :
B 21.08 [0.05] D 2007MNRAS.379.1117R
V 20.16 [0.05] D 2007MNRAS.379.1117R
R 19.53 [0.05] D 2007MNRAS.379.1117R
G 20.172272 [0.024249] C 2020yCat.1350....0G
I 18.79 [0.05] D 2007MNRAS.379.1117R
K 17.8 [0.1] D 2007MNRAS.379.1117R
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Identifiers (12) :
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PSR J1959+2048 3FGL J1959.5+2047 NAME PSR B1957+20 b EQ J195936+204814
1FGL J1959.6+2047 4FGL J1959.5+2048 PSR B1957+20 Gaia DR3 1823773960079216896
2FGL J1959.5+2047 NAME Black Widow V* QX Sge Gaia DR2 1823773960079216896

References (854 between 1850 and 2026) (Total 854)
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

Plx : 1    PM : 2    SpT : 1   

   

Observing logs
XMM : 1   

   


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Link by name to the catalogue in VizieR :

V* QX Sge Gaia DR3 1823773960079216896 Gaia DR2 1823773960079216896

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