MURAL - Maynooth University Research Archive Library

    A search for the optical counterpart of PSR B1951+32 in the supernova remnant CTB 80

    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

    Download (177kB) | Preview

    Share your research

    Twitter Facebook LinkedIn GooglePlus Email more...

    Add this article to your Mendeley library


    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

    Repository Staff Only(login required)

    View Item Item control page


    Downloads per month over past year