2003A&A...397..969K


C.D.S. - SIMBAD4 rel 1.7 - 2020.11.28CET00:22:31

2003A&A...397..969K - Astronomy and Astrophysics, volume 397, 969-972 (2003/1-3)

Radio emission altitude in pulsars.

KIJAK J. and GIL J.

Abstract (from CDS):

The method of emission altitude estimation in radio pulsars based on pulse width measurements at the low intensity profile wings is reviewed. Both measurement details and model assumptions are discussed. It is argued that the pulse width measurement technique is sensitive enough to detect the radio emission generated at the beam edge near the last open field lines. We give the refined version of the formula for the radio emission altitudes and compare it with values obtained independently using a method based on measurements of separation between peaks of the outermost profile components. We show that both methods give comparable results.

Abstract Copyright:

Journal keyword(s): stars: pulsars: general

Simbad objects: 7

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Number of rows : 7

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 PSR B0301+19 Psr 03 04 33.115 +19 32 51.40           ~ 203 0
2 PSR B0329+54 Psr 03 32 59.3462817079 +54 34 45.047901390           ~ 582 1
3 PSR B0525+21 Psr 05 28 52.308 +22 00 01.00           ~ 326 0
4 PSR B1133+16 Psr 11 36 03.180 +15 51 09.62           ~ 613 0
5 PSR B1237+25 Psr 12 39 40.386 +24 53 49.87           ~ 414 0
6 PSR B2020+28 Psr 20 22 37.0671 +28 54 23.104           ~ 282 1
7 PSR B2045-16 Psr 20 48 35.446 -16 16 43.00           ~ 286 0

    Equat.    Gal    SGal    Ecl

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2020.11.28-00:22:31

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