1997A&A...321..519S


Query : 1997A&A...321..519S

1997A&A...321..519S - Astronomy and Astrophysics, volume 321, 519-522 (1997/5-2)

Geometrical effects on radio pulsar profiles and spectra.

SIEBER W.

Abstract (from CDS):

Considering the geometry of the hollow-cone model of radio pulsar emission in detail, one is led to the conclusion that several well-known observed effects may be explained quite easily purely on geometrical terms. It can be shown e.g. that the appearance of outriders at high frequencies and a steepening of the whole spectrum (cut-off) must be expected for certain geometrical situations as well as variations in component spectra, e.g. a steepening of the central (core) component. These effects appear in addition to the presumably also existing physical variations with frequency.

Abstract Copyright:

Journal keyword(s): pulsars: general - radiation mechanisms: general

Simbad objects: 8

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Number of rows : 8
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 PSR B0525+21 Psr 05 28 52.308 +22 00 01.00     14.30     ~ 356 0
2 PSR B0950+08 Psr 09 53 09.2970 +07 55 36.400           ~ 755 2
3 PSR B1133+16 Psr 11 36 03.0720 +15 51 15.500           ~ 668 0
4 PSR B1237+25 Psr 12 39 40.386 +24 53 49.87           ~ 468 0
5 PSR B1642-03 Psr 16 45 02.0330 -03 17 57.200           ~ 363 0
6 PSR B1749-28 Psr 17 52 58.7130 -28 06 33.900           ~ 261 0
7 PSR B1933+16 Psr 19 35 47.7011639352 +16 16 40.034899524           ~ 302 1
8 PSR B2016+28 Psr 20 18 03.8999255016 +28 39 54.940329468           ~ 356 0

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