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  Timing and Interstellar Scattering of Thirty-five Distant Pulsars Discovered in the PALFA Survey

Nice, D. J., Altiere, E., Bogdanov, S., Cordes, J. M., Farrington, D., Hessels, J. W. T., et al. (2013). Timing and Interstellar Scattering of Thirty-five Distant Pulsars Discovered in the PALFA Survey. Astrophysical Journal, 772: 50. doi:10.1088/0004-637X/772/1/50.

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 Urheber:
Nice, D. J., Autor
Altiere, E., Autor
Bogdanov, S., Autor
Cordes, J. M., Autor
Farrington, D., Autor
Hessels, J. W. T., Autor
Kaspi, V. M., Autor
Lyne, A. G., Autor
Popa, L., Autor
Ransom, S. M., Autor
Sanpa-arsa, S., Autor
Stappers, B. W., Autor
Wang, Y., Autor
Allen, B.1, Autor           
Bhat, N. D. R., Autor
Brazier, A., Autor
Camilo, F., Autor
Champion, D. J., Autor
Chatterjee, S., Autor
Crawford, F., Autor
Deneva, J. S., AutorDesvignes, G., AutorFreire, P. C. C., AutorJenet, F. A., AutorKnispel, B.1, Autor           Lazarus, P., AutorLee, K. J., Autorvan Leeuwen, J., AutorLorimer, D. R., AutorLynch, R., AutorMcLaughlin, M. A., AutorScholz, P., AutorSiemens, X., AutorStairs, I. H., AutorStovall, K., AutorVenkataraman, A., AutorZhu, W., Autor mehr..
Affiliations:
1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              

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Schlagwörter: Astrophysics, Solar and Stellar Astrophysics, astro-ph.SR, Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE
 Zusammenfassung: We 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. Lastly, 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.

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 Datum: 2013-04-272013-07-072013
 Publikationsstatus: Erschienen
 Seiten: Published in the Astrophysical Journal
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: -
 Identifikatoren: arXiv: 1304.7370
DOI: 10.1088/0004-637X/772/1/50
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Titel: Astrophysical Journal
Genre der Quelle: Zeitschrift
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Ort, Verlag, Ausgabe: Chicago, IL : University of Chicago Press for the American Astronomical Society
Seiten: - Band / Heft: 772 Artikelnummer: 50 Start- / Endseite: - Identifikator: ISSN: 0004-637X
CoNE: https://pure.mpg.de/cone/journals/resource/954922828215_2