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Volumn , Issue , 2008, Pages 1-504

Astrophysics processes: The physics of astronomical phenomena

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[No Author keywords available]

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EID: 84924164949     PISSN: None     EISSN: None     Source Type: Book    
DOI: 10.1017/CBO9780511802249     Document Type: Book
Times cited : (32)

References (54)
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    • Cosmology with the s-z effect
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    • Carlstrom, J.1    Holder, G.2    Reese, E.3
  • 26
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    • High-resolution optical and ultraviolet absorption-line studies of the interstellar gas
    • L. Cowie and A. Songaila, “High-resolution optical and ultraviolet absorption-line studies of the interstellar gas,” ARAA 24, 499 (1986) (10).
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  • 27
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    • The three-phase interstellar medium revisited
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    • Cox, D.1
  • 28
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    • The supermassive black hole at the galactic center
    • F. Melia and H. Falcke, “The supermassive black hole at the galactic center,” ARAA 39, 309 (2001) (1).
    • (2001) ARAA , vol.39 , Issue.1 , pp. 309
    • Melia, F.1    Falcke, H.2
  • 30
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    • Weak gravitational lensing by large-scale structure
    • A Refregier, “Weak gravitational lensing by large-scale structure,” ARAA 41, 645 (2003) (12).
    • (2003) ARAA , vol.41 , Issue.12 , pp. 645
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    • X-ray properties of black-hole binaries
    • R. Remillard and J. McClintock, “X-ray properties of black-hole binaries,” ARAA 44, 49 (2006) (4).
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    • Remillard, R.1    McClintock, J.2
  • 32
    • 0036404940 scopus 로고    scopus 로고
    • The evolution of x-ray clusters of galaxies
    • P. Rosati, S. Borgani, and C. Norman, “The evolution of x-ray clusters of galaxies,” ARAA 40, 539 (2002) (9).
    • (2002) ARAA , vol.40 , Issue.9 , pp. 539
    • Rosati, P.1    Borgani, S.2    Norman, C.3
  • 33
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    • Rotation curves of spiral galaxies
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  • 34
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    • Formation and evolution of compact stellar x-ray sources
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    • Review articles in the Annual Review of Astronomy and Astrophysics; each volume contains a list of titles of the previous dozen or so volumes Articles in amateur astronomy magazines such as Sky and Telescope (see “News Notes”) and Astronomy.
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.