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Volumn 307, Issue 5711, 2005, Pages 892-896

Twenty-one millisecond pulsars in Terzan 5 using the Green Bank Telescope

Author keywords

[No Author keywords available]

Indexed keywords

CONSTRAINT THEORY; EQUATIONS OF STATE; SUN; TELESCOPES;

EID: 13644267184     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1108632     Document Type: Article
Times cited : (324)

References (48)
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    • (1992)
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    • note
    • The core radius is defined as that where the optical surface brightness is half its central value.
  • 10
    • 13644251835 scopus 로고    scopus 로고
    • F. Piotto, G. Meylan, S. G. Djorgovski, M. Riello, Eds. [Astronomical Society of the Pacific (ASP) Conference Series no. 296, ASP, San Francisco, CA, 2003]
    • F. Verbunt, in New Horizons in Globular Cluster Astronomy, F. Piotto, G. Meylan, S. G. Djorgovski, M. Riello, Eds. [Astronomical Society of the Pacific (ASP) Conference Series no. 296, ASP, San Francisco, CA, 2003], p. 245.
    • New Horizons in Globular Cluster Astronomy , pp. 245
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    • F. van Leeuwen, J. D. Hughes, F. Piotto, Eds. ASP Conference Series no. 265, ASP, San Francisco, CA
    • F. Verbunt, in Omega Centauri, A Unique Window into Astrophysics, F. van Leeuwen, J. D. Hughes, F. Piotto, Eds. (ASP Conference Series no. 265, ASP, San Francisco, CA, 2002), p. 289.
    • (2002) Omega Centauri, A Unique Window into Astrophysics , pp. 289
    • Verbunt, F.1
  • 18
    • 13644252538 scopus 로고    scopus 로고
    • note
    • The 442-ms pulsar J1748-2444 was initially identified as Ter 5 B (B1744-24B) but is now known to be a foreground pulsar unrelated to Terzan 5 (20).
  • 19
    • 0009278078 scopus 로고
    • A. G. Lyne et al., Nature 347, 650 (1990).
    • (1990) Nature , vol.347 , pp. 650
    • Lyne, A.G.1
  • 21
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    • thesis, Harvard University, Cambridge, MA
    • S. M. Ransom, thesis, Harvard University, Cambridge, MA (2001).
    • (2001)
    • Ransom, S.M.1
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    • note
    • The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Incorporated.
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    • in preparation
    • D. Kaplan et al., in preparation.
    • Kaplan, D.1
  • 26
    • 13644268835 scopus 로고    scopus 로고
    • note
    • These comparisons assume a typical pulsar spectral index of -1.6 (32).
  • 29
    • 13644252537 scopus 로고    scopus 로고
    • note
    • Ter 5 E was a candidate (i.e., unconfirmed) pulsar in (21).
  • 35
    • 13644265890 scopus 로고    scopus 로고
    • note
    • 1950,min is about 8 μJy for P ∼ 2- to 4-ms isolated or long orbital period MSPs.
  • 39
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    • F. Rasio, I. Stairs, Eds. (ASP Conference Series no. 328, ASP, San Francisco, CA)
    • A. Possenti et al., in Binary Radio Pulsars, F. Rasio, I. Stairs, Eds. (ASP Conference Series no. 328, ASP, San Francisco, CA, 2005), p. 189.
    • (2005) Binary Radio Pulsars , pp. 189
    • Possenti, A.1
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    • F. Rasio, I. Stairs, Eds. (ASP Conference Series no. 328, ASP, San Francisco, CA)
    • D. J. Nice, E. M. Splaver, I. H. Stairs, in Binary Radio Pulsars, F. Rasio, I. Stairs, Eds. (ASP Conference Series no. 328, ASP, San Francisco, CA, 2005), p. 371.
    • (2005) Binary Radio Pulsars , pp. 371
    • Nice, D.J.1    Splaver, E.M.2    Stairs, I.H.3
  • 47
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    • The Tempo program is available online at http://pulsar.princeton.edu/ tempo.
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    • note
    • We thank F. Rasio, S. Sigurdsson, and M. van Kerkwijk for extremely useful discussions and J. Herrnstein, L. Greenhill, D. Manchester, A. Lyne, and N. D'Amico for providing or aiding with the Parkes data from 1998 and 2000. J.W.T.H. is a Natural Sciences and Engineering Research Council of Canada (NSERC) Post-Graduate Scholarship-Doctoral fellow. I.H.5. holds an NSERC University Faculty Award and is supported by a Discovery grant and University of British Columbia start-up funds. F.C. thanks support from NSF. V.M.K. holds a Canada Research Chair and is supported by an NSERC Discovery Grant and Steacie Fellowship Supplement, by the Fonds Québécois de la recherche sur la nature et les technologies and Canadian Institute for Advanced Research, and by a New Opportunities Grant from the Canada Foundation for Innovation. D.L.K. is a Pappalardo Fellow.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.