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Volumn 422, Issue 3, 2004, Pages 915-923

A variable ultra-luminous X-ray source in the colliding galaxy NGC 7714

Author keywords

Accretion, accretion disks; Black hole physics; Galaxies: Individual: NGC 7714; X ray: Stars; X rays: Galaxies

Indexed keywords

DATA REDUCTION; KINEMATICS; LUMINOUS MATERIALS; PARAMETER ESTIMATION; RADIATION; SURFACE TREATMENT; X RAY ANALYSIS; X RAYS;

EID: 3442889494     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040265     Document Type: Article
Times cited : (22)

References (70)
  • 1
    • 0003123372 scopus 로고    scopus 로고
    • Astronomical data analysis software and systems V
    • ed. G. Jacoby G., & J. Barnes
    • Arnaud, K. A. 1996, Astronomical Data Analysis Software and Systems V, ed. G. Jacoby G., & J. Barnes, ASP Conf. S er., 101, 17
    • (1996) ASP Conf. Ser. , vol.101 , pp. 17
    • Arnaud, K.A.1
  • 21
  • 25
    • 3442886102 scopus 로고    scopus 로고
    • The Restless High-Energy Universe (Amsterdam, May 2003), ed. E. P. J. van den Heuvel, J. J. M. in't Zand, & R. A. M. J. Wijers, in press [arXiv:astro-ph/0309725]
    • Gilfanov, M., Grimm, H.-J., & Sunyaev, R. 2003, Proc. BeppoSAX Symp., The Restless High-Energy Universe (Amsterdam, May 2003), ed. E. P. J. van den Heuvel, J. J. M. in't Zand, & R. A. M. J. Wijers, in press [arXiv:astro-ph/0309725]
    • (2003) Proc. BeppoSAX Symp.
    • Gilfanov, M.1    Grimm, H.-J.2    Sunyaev, R.3
  • 32
    • 0042916908 scopus 로고
    • Higdon, J. L. 1995, ApJ, 455, 524
    • (1995) ApJ , vol.455 , pp. 524
    • Higdon, J.L.1
  • 52
    • 0142041893 scopus 로고    scopus 로고
    • Read, A. M. 2003, MNRAS, 342, 715
    • (2003) MNRAS , vol.342 , pp. 715
    • Read, A.M.1
  • 58
  • 62
    • 0000297077 scopus 로고
    • Toomre, A. 1977, ARA&A, 15, 437
    • (1977) ARA&A , vol.15 , pp. 437
    • Toomre, A.1
  • 66
    • 0001454411 scopus 로고    scopus 로고
    • Wang, Q. D. 2002, MNRAS, 332, 764
    • (2002) MNRAS , vol.332 , pp. 764
    • Wang, Q.D.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.