2004ApJ...609..335G


Query : 2004ApJ...609..335G

2004ApJ...609..335G - Astrophys. J., 609, 335-339 (2004/July-1)

Pulsar radio emission altitude from curvature radiation.

GANGADHARA R.T.

Abstract (from CDS):

We assume that relativistic sources moving along dipolar magnetic field lines emit curvature radiation. The beamed emission occurs in the direction of tangents to the field lines, and to receive it, the sight line must align with the tangent within the beaming angle 1/γ, where γ is the particle Lorentz factor. By solving the viewing geometry in an inclined and rotating dipolar magnetic field, we show that at any given pulse phase, the observer tends to receive radiation only from the specific heights allowed by the geometry. We find that outer conal components are emitted at higher altitudes compared to inner components, including the core. At any pulse phase, low-frequency emission comes from higher altitudes than high-frequency emission. We have modeled the emission heights of pulse components of PSR B0329+54 and estimated field line curvature radii and particle Lorentz factors in the emission regions.

Abstract Copyright: ∼

Journal keyword(s): Stars: Pulsars: General - Stars: Pulsars: Individual: Alphanumeric: PSR B0329+54 - Radio Continuum: Stars - Stars: Magnetic Fields

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 B0329+54 Psr 03 32 59.3370698592 +54 34 45.028206408           ~ 690 1

Query : 2004ApJ...609..335G

Basic data :
PSR B0329+54 -- Pulsar
Other object types:
otypes_help
Rad (GB6,MY,...), Psr (PSR,PULS), * (Gaia), NIR (2MASS)
ICRS coord. (ep=J2000) :
03 32 59.3370698592 +54 34 45.028206408 (Optical) [ 0.4683 0.4608 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
03 29 11.0039353995 +54 24 38.968936308 [ 0.4683 0.4608 90 ]
Gal coord. (ep=J2000) :
144.9949679143101 -01.2203063262975 [ 0.4683 0.4608 90 ]
Proper motions mas/yr :
5.020 -2.503 [0.582 0.657 90] A 2020yCat.1350....0G
Parallaxes (mas):
0.209 [0.6583] A 2020yCat.1350....0G
Fluxes (4) :
G 20.136793 [0.006418] C 2020yCat.1350....0G
J 17.093 [0.193] D 2003yCat.2246....0C
H 16.183 [0.203] D 2003yCat.2246....0C
K 15.556 [0.172] D 2003yCat.2246....0C
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1
Display criteria :

Identifiers (16) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

PSR B0329+54 NVSS J033259+543444 TGSSADR J033259.1+543442 WN B0329.1+5424
GB6 B0329+5425 PSR J0332+5434 TIC 316847481 WSTB 32W244
2MASS J03325936+5434448 PULS CP 0329 TXS 0329+544 Gaia DR2 445135392719883904
MY 032910.9+543447.0 PULS CP 0328 WN J0332+5434 Gaia DR3 445135392719883904

References (690 between 1850 and 2026) (Total 690)
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

Distance : 1    Plx : 3    PM : 3   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : PSR B0329+54

Link by name to the catalogue in VizieR :

2MASS J03325936+5434448 NVSS J033259+543444 WN J0332+5434 WN B0329.1+5424 Gaia DR2 445135392719883904
Gaia DR3 445135392719883904

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