O'Sullivan, Créidhe and Shearer, A. and Colhoun, M. and Golden, A. and Redfern, M. and Butler, R. and Beskin, G.M. and Niezvestny, S.I. and Neustroev, V.V. and Plokhotnichenko, V.L. and Danks, A.
(1998)
A search for the optical counterpart of PSR B1951+32
in the supernova remnant CTB 80.
Astronomy and Astrophysics, 335.
pp. 991-994.
ISSN 0004-6361
Abstract
Using time-resolved two-dimensional aperture photometry
we have put upper limits on the pulsed emission from
two proposed optical counterparts for PSR B1951+32. Our
pulsed upper limits of mv,pulsed > 23.3, mb,pulsed > 24.4,
for the first candidate and mv,pulsed > 23.6, mb,pulsed > 24.3
for the second, make it unlikely that either of these is, in fact,
the pulsar. We discuss three further candidates, but also reject
these on the basis of timing results. A search of a 5.""5 × 5.""5
area centred close to these stars failed to find any significant
pulsations at the reported pulsar period.
Item Type: |
Article
|
Keywords: |
pulsars; individual; PSR B1951+32 – ISM; individual
objects; CTB 80; |
Academic Unit: |
Faculty of Science and Engineering > Experimental Physics |
Item ID: |
7101 |
Depositing User: |
Dr. Créidhe O'Sullivan
|
Date Deposited: |
05 May 2016 14:53 |
Journal or Publication Title: |
Astronomy and Astrophysics |
Publisher: |
EDP Sciences |
Refereed: |
Yes |
URI: |
|
Use Licence: |
This item is available under a Creative Commons Attribution Non Commercial Share Alike Licence (CC BY-NC-SA). Details of this licence are available
here |
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