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dc.contributor.authorPopa, Laura Cornelia
dc.date.accessioned2015-01-29T17:58:28Z
dc.date.available2015-01-29T17:58:28Z
dc.date.issued2013-07
dc.date.submitted2013-04
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttp://hdl.handle.net/1721.1/93199
dc.description.abstractWe have made extensive observations of 35 distant slow (non-recycled) pulsars discovered in the ongoing Arecibo PALFA pulsar survey. Timing observations of these pulsars over several years at Arecibo Observatory and Jodrell Bank Observatory have yielded high-precision positions and measurements of rotation properties. Despite being a relatively distant population, these pulsars have properties that mirror those of the previously known pulsar population. Many of the sources exhibit timing noise, and one underwent a small glitch. We have used multifrequency data to measure the interstellar scattering properties of these pulsars. We find scattering to be higher than predicted along some lines of sight, particularly in the Cygnus region. Finally, we present XMM-Newton and Chandra observations of the youngest and most energetic of the pulsars, J1856+0245, which has previously been associated with the GeV-TeV pulsar wind nebula HESS J1857+026.en_US
dc.language.isoen_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/0004-637X/772/1/50en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAmerican Astronomical Societyen_US
dc.titleTIMING AND INTERSTELLAR SCATTERING OF 35 DISTANT PULSARS DISCOVERED IN THE PALFA SURVEYen_US
dc.typeArticleen_US
dc.identifier.citationNice, D. J., E. Altiere, S. Bogdanov, J. M. Cordes, D. Farrington, J. W. T. Hessels, V. M. Kaspi, et al. “TIMING AND INTERSTELLAR SCATTERING OF 35 DISTANT PULSARS DISCOVERED IN THE PALFA SURVEY.” The Astrophysical Journal 772, no. 1 (July 5, 2013): 50. © 2013 The American Astronomical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.mitauthorPopa, Laura Corneliaen_US
dc.relation.journalAstrophysical Journalen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsNice, D. J.; Altiere, E.; Bogdanov, S.; Cordes, J. M.; Farrington, D.; Hessels, J. W. T.; Kaspi, V. M.; Lyne, A. G.; Popa, L.; Ransom, S. M.; Sanpa-arsa, S.; Stappers, B. W.; Wang, Y.; Allen, B.; Bhat, N. D. R.; Brazier, A.; Camilo, F.; Champion, D. J.; Chatterjee, S.; Crawford, F.; Deneva, J. S.; Desvignes, G.; Freire, P. C. C.; Jenet, F. A.; Knispel, B.; Lazarus, P.; Lee, K. J.; van Leeuwen, J.; Lorimer, D. R.; Lynch, R.; McLaughlin, M. A.; Scholz, P.; Siemens, X.; Stairs, I. H.; Stovall, K.; Venkataraman, A.; Zhu, W.en_US
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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