PSR 0540-693

Andrew Shearer

PSR 0540-693

Andrew Shearer

Physics

Research output: Contribution to a Journal (Peer & Non Peer) › Article › peer-review

Abstract

A. Shearer, M. Redfern, T. Rowold, P. OKane, R. Butler, and C. OByrne, University College, Galway; and H. Pedersen, Copenhagen University Observatory, communicate: We have observed the position of the optical pulsar 0540-693 (Middleditch and Pennypacker 1985, Nature, 313, 659) using the European Southern Observatorys New Technology Telescope (+ UCG DIAS ESO MAMA image sharpening camera, TRIFFID) on 1993 Jan. 15-16. On each night, the 19.838-Hz barycentric power spectrum component (computed from the pulsar period given in Manchester et al. (1993, Ap.J. 403, L103) showed a single spatial peak, consistent in height with Middleditch and Pennypacker, in the center of the nebulosity and coincident with the northern maximum of Caraveo et al. (1992, Ap.J. 395, L103).

Original language	English (Ireland)
Number of pages	2
Journal	\iaucirc
Volume	5786
Publication status	Published - 1 May 1993

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Authors
Shearer

Cite this

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title = "PSR 0540-693",

abstract = "A. Shearer, M. Redfern, T. Rowold, P. OKane, R. Butler, and C. OByrne, University College, Galway; and H. Pedersen, Copenhagen University Observatory, communicate: We have observed the position of the optical pulsar 0540-693 (Middleditch and Pennypacker 1985, Nature, 313, 659) using the European Southern Observatorys New Technology Telescope (+ UCG DIAS ESO MAMA image sharpening camera, TRIFFID) on 1993 Jan. 15-16. On each night, the 19.838-Hz barycentric power spectrum component (computed from the pulsar period given in Manchester et al. (1993, Ap.J. 403, L103) showed a single spatial peak, consistent in height with Middleditch and Pennypacker, in the center of the nebulosity and coincident with the northern maximum of Caraveo et al. (1992, Ap.J. 395, L103). ",

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N2 - A. Shearer, M. Redfern, T. Rowold, P. OKane, R. Butler, and C. OByrne, University College, Galway; and H. Pedersen, Copenhagen University Observatory, communicate: We have observed the position of the optical pulsar 0540-693 (Middleditch and Pennypacker 1985, Nature, 313, 659) using the European Southern Observatorys New Technology Telescope (+ UCG DIAS ESO MAMA image sharpening camera, TRIFFID) on 1993 Jan. 15-16. On each night, the 19.838-Hz barycentric power spectrum component (computed from the pulsar period given in Manchester et al. (1993, Ap.J. 403, L103) showed a single spatial peak, consistent in height with Middleditch and Pennypacker, in the center of the nebulosity and coincident with the northern maximum of Caraveo et al. (1992, Ap.J. 395, L103).

AB - A. Shearer, M. Redfern, T. Rowold, P. OKane, R. Butler, and C. OByrne, University College, Galway; and H. Pedersen, Copenhagen University Observatory, communicate: We have observed the position of the optical pulsar 0540-693 (Middleditch and Pennypacker 1985, Nature, 313, 659) using the European Southern Observatorys New Technology Telescope (+ UCG DIAS ESO MAMA image sharpening camera, TRIFFID) on 1993 Jan. 15-16. On each night, the 19.838-Hz barycentric power spectrum component (computed from the pulsar period given in Manchester et al. (1993, Ap.J. 403, L103) showed a single spatial peak, consistent in height with Middleditch and Pennypacker, in the center of the nebulosity and coincident with the northern maximum of Caraveo et al. (1992, Ap.J. 395, L103).

M3 - Article

VL - 5786

JO - \iaucirc

JF - \iaucirc

ER -

PSR 0540-693

Abstract

Authors (Note for portal: view the doc link for the full list of authors)

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