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Volumn 417, Issue 3, 2004, Pages 853-871

Probing the cosmological variation of the fine-structure constant: Results based on VLT-UVES sample

Author keywords

Cosmology: observations; Galaxies: quasars: absorption lines

Indexed keywords

ABSORPTION; ASTROPHYSICS; ATOMIC PHYSICS; COMPUTER SIMULATION; GALAXIES; MATHEMATICAL MODELS; SIGNAL TO NOISE RATIO; SPURIOUS SIGNAL NOISE;

EID: 2442607147     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20035701     Document Type: Article
Times cited : (244)

References (34)
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    • Ashenfelter, T., Mathews, G. J., & Olive, K. A. 2003 [astro-ph/0309197]
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    • Chengalur, J. N., & Kanekar, N. 2003 [astro-ph/0310764]
    • Chengalur, J. N., & Kanekar, N. 2003 [astro-ph/0310764]
  • 16
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    • Morton, D. C. 1991, ApJS, 77, 119
    • (1991) ApJS , vol.77 , pp. 119
    • Morton, D.C.1
  • 17
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    • Morton, D. C. 1992, ApJS, 81, 883
    • (1992) ApJS , vol.81 , pp. 883
    • Morton, D.C.1
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    • Uzan, J. 2003, RvMP, 75, 403
    • (2003) RvMP , vol.75 , pp. 403
    • Uzan, J.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.