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Volumn 330, Issue 6008, 2010, Pages 1209-1212

A magnetized jet from a massive protostar

Author keywords

[No Author keywords available]

Indexed keywords

ASTROPHYSICS; JET; MAGNETIC FIELD;

EID: 78649407197     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1195589     Document Type: Article
Times cited : (216)

References (42)
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    • note
    • This scenario is well stablished in the case of low-mass stars, whereas for high-mass stars the evidence of disk/jet systems is more scarce [e.g., (40)].
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    • 0007114947 scopus 로고    scopus 로고
    • D. T. Wickramasinghe, L. Ferrario, G. V. Bicknell, Eds. ASP Conference Series Astronomical Society of the Pacific, San Francisco
    • M. Livio, in Accretion Phenomena and Related Outflows, IAU Colloquium 163, D. T. Wickramasinghe, L. Ferrario, G. V. Bicknell, Eds. (ASP Conference Series Vol. 121, Astronomical Society of the Pacific, San Francisco, 1997), pp. 845-866.
    • (1997) Accretion Phenomena and Related Outflows, IAU Colloquium , vol.121-163 , pp. 845-866
    • Livio, M.1
  • 9
    • 33947647697 scopus 로고    scopus 로고
    • B. Reipurth, D. Jewitt, K. Keil, Eds. University of Arizona Press, Tucson, AZ
    • R. E. Pudritz, R. Ouyed, Ch. Fendt, A. Brandenburg, in Protostars and Planets V, B. Reipurth, D. Jewitt, K. Keil, Eds. (University of Arizona Press, Tucson, AZ, 2007), pp. 277-294.
    • (2007) Protostars and Planets V , pp. 277-294
    • Pudritz, R.E.1    Ouyed, R.2    Fendt, Ch.3    Brandenburg, A.4
  • 15
  • 22
    • 78649473515 scopus 로고    scopus 로고
    • note
    • Circularly polarized emission has been reported in the ejecta of the young star T Tauri South (41), but in this case the proposed mechanism is gyrosynchrotron, which has different polarization characteristics than synchrotron and is expected to be relevant only close to the stellar surfaces.
  • 24
    • 78649459742 scopus 로고    scopus 로고
    • See supporting material on Online
    • See supporting material on Science Online.
    • Science
  • 40
    • 27744465971 scopus 로고    scopus 로고
    • N. A. Patel et al., Nature 437, 109 (2005).
    • (2005) Nature , vol.437 , pp. 109
    • Patel, N.A.1
  • 41
    • 0031013869 scopus 로고    scopus 로고
    • T. P. Ray et al., Nature 385, 415 (1997).
    • (1997) Nature , vol.385 , pp. 415
    • Ray, T.P.1
  • 42
    • 78649453398 scopus 로고    scopus 로고
    • note
    • National Radio Astronomy Observatory is a facility of the NSF, operated under cooperative agreement by Associated Universities, Incorporated. We acknowledge I. Agudo, A. Alberdi, and J. L. Gómez for useful comments. G.A., C.C.-G., J.M., M.O., and J.M.T. acknowledge support from Ministerio de Ciencia e Innovación (Spain) grants AYA2008-06189-C03 and AYA2007-68034-C03-02 [co-funded with Fondo Europeo de Desarrollo Regional (FEDER) funds] and from Junta de Andalucía (Spain). L.F.R. acknowledges the support of Dirección General de Asuntos del Personal Académico, UNAM, and Consejo Nacional de Ciencia y Technología, México.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.