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Volumn 366, Issue 3, 2006, Pages 1096-1117

Resolving the kinematic distance ambiguity of southern massive young stellar object candidates

Author keywords

Galaxy: structure; ISM: kinematics and dynamics

Indexed keywords

STARS; SURVEYS;

EID: 33645068177     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09909.x     Document Type: Article
Times cited : (55)

References (28)
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    • Flynn, E.S.1    Jackson, J.M.2    Simon, R.3    Shah, R.Y.4    Bania, T.5
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    • Hoare, M.G.1    Lumsden, S.L.2    Oudmaijer, R.D.3    Busfield, A.L.4    King, T.L.5    Moore, T.L.J.6
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    • Taylor A. R., Stil J. M., Dickey J. M., McClure-Griffiths N. M., Martin P. G., Rothwell T., Lockman F. J., 2002, in Taylor A. R., Landecker T. L., Willis A. G., eds, ASP Conf. Ser. Vol. 276, Seeing Through the Dust: the Detection of H I and the Exploration of the ISM in Galaxies. Astron. Soc. Pac., San Francisco, p. 68
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    • Taylor, A.R.1    Stil, J.M.2    Dickey, J.M.3    McClure-Griffiths, N.M.4    Martin, P.G.5    Rothwell, T.6    Lockman, F.J.7


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.