2001MNRAS.325..187L


Query : 2001MNRAS.325..187L

2001MNRAS.325..187L - Mon. Not. R. Astron. Soc., 325, 187-196 (2001/July-3)

Cyclotron absorption of radio emission within pulsar magnetospheres.

LUO Q. and MELROSE D.B.

Abstract (from CDS):

Absorption of radio emission through normal cyclotron resonance within pulsar magnetospheres is considered. The optical depth for cyclotron damping is calculated using a plasma distribution with an intrinsically relativistic spread. We argue that such a broad distribution is plausible for pulsar plasmas and that it implies that a class of pulsars that should have cyclotron damping extends to include young pulsars with shorter periods and stronger magnetic fields. There is no obvious observational evidence for disruption of radio pulses, which implies that the optical depth cannot be too large. We propose that cyclotron resonance may cause marginal absorption of radio emission. It is shown that such marginal absorption produces potentially observable asymmetric features for double-peak pulse profiles with wide separation, with one peak tending to be suppressed.

Abstract Copyright: The Royal Astronomical Society

Journal keyword(s): acceleration of particles - radiation mechanisms: non-thermal - pulsars: general

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 J1549-4848 Psr 15 49 21.02700 -48 48 36.1000           ~ 55 0

Query : 2001MNRAS.325..187L

Basic data :
PSR J1549-4848 -- Pulsar
Other object types:
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Psr (PSR)
ICRS coord. (ep=J2000) :
15 49 21.02700 -48 48 36.1000 (Radio) [ 61 100 90 ] B 2020MNRAS.494..228L
FK4 coord. (ep=B1950 eq=1950) :
15 45 43.46563 -48 39 28.3600 [ 61 100 90 ]
Gal coord. (ep=J2000) :
330.49437684 +04.30451754 [ 61 100 90 ]
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Identifiers (1) :
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PSR J1549-4848

References (55 between 1850 and 2026) (Total 55)
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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