SIMBAD references

2008MNRAS.386.1411B - Mon. Not. R. Astron. Soc., 386, 1411-1416 (2008/May-3)

The expansion and radio spectral index of G21.5-0.9: is PSR J1833-1034 the youngest pulsar?

BIETENHOLZ M.F. and BARTEL N.

Abstract (from CDS):

We report on new 5-GHz Very Large Array (VLA) radio observations of the pulsar-powered supernova remnant G21.5-0.9. These observations have allowed us to make a high-quality radio image of this remnant with a resolution of ∼0.7 arcsec. It has a filamentary structure similar to that seen in the Crab Nebula. Radio structure suggestive of the torus seen around the Crab pulsar is tentatively identified. We also compared the new image with one taken ∼15 yr earlier at 1.5 GHz, both to find the expansion speed of the remnant and to make a spectral index image. Between 1991 and 2006, we find that the average expansion rate of the remnant is 0.11±0.02 per cent/yr, corresponding, for a distance of 5 kpc, to a speed of 910±160km/s with respect to the centre of the nebula. Assuming undecelerated expansion, this expansion speed implies that the age of G21.5-0.9 is 870+200–150yr, which makes PSR J1833-1034 one of the youngest, if not the youngest, known pulsars in the Galaxy.

Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): supernova remnants

Simbad objects: 10

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2008MNRAS.386.1411B and select 'bookmark this link' or equivalent in the popup menu


2021.03.04-13:00:42

© Université de Strasbourg/CNRS

    • Contact